This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp
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 09 19.3738 2461302.8738 12.88 03:30:41.74 +18:27:58.0
167.61386 -30.26439 galactic Tau Second-epoch detections are separated by 0.5" 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.72 Feronia -0 -0 0 12.8 -0 0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:30:41.74 +18:27:58.0: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:30:41.74 +18:27:58.0: 16.18 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 19.3738* 03 30 41.74 +18 27 58.0 12.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8738,12.88,0.05,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 20260919.3738 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 19.3738 2461302.8738 13.27 04:05:03.15 +17:55:18.2
174.63474 -24.95213 galactic Tau Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.62 Erato 1 0 1 13.5 -0 0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 04:05:03.15 +17:55:18.2: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 04:05:03.15 +17:55:18.2: 15.89 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 19.3738* 04 05 03.15 +17 55 18.2 13.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8738,13.27,0.05,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 20260919.3738 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 19.3738 2461302.8738 13.54 03:06:07.85 +16:20:01.8
163.82235 -35.62858 galactic Ari Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.149 Medusa -0 -0 1 13.7 0 0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:06:07.85 +16:20:01.8: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:06:07.85 +16:20:01.8: 15.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 19.3738* 03 06 07.85 +16 20 01.8 13.5 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8738,13.54,0.05,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 20260919.3738 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 19.3738 2461302.8738 13.76 03:18:27.84 +10:16:18.3
171.58377 -38.33864 galactic Cet Second-epoch detections are separated by 0.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.619 Triberga 0 -0 0 13.8 -0 0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:18:27.84 +10:16:18.3: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:18:27.84 +10:16:18.3: 16.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 19.3738* 03 18 27.84 +10 16 18.3 13.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8738,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260919.3738 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 19.3738 2461302.8738 13.78 03:55:13.96 +16:23:56.2
174.07856 -27.70388 galactic Tau Second-epoch detections are separated by 0.5" 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.443 Photographica -1 -2 2 14.1 -0 -0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:55:13.96 +16:23:56.2: 16.08 +/- 0.35 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:55:13.96 +16:23:56.2: 16.09 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 16.08 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 19.3738* 03 55 13.96 +16 23 56.2 13.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8738,13.78,0.05,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 20260919.3738 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 19.3738 2461302.8738 14.21 03:50:22.02 +17:07:13.6
172.57445 -28.03436 galactic Tau Second-epoch detections are separated by 1.3" 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.131 Vala -0 0 0 14.6 -0 -0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:50:22.02 +17:07:13.6: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:50:22.02 +17:07:13.6: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 19.3738* 03 50 22.02 +17 07 13.6 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8738,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260919.3738 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 19.3738 2461302.8738 14.29 03:59:31.69 +15:00:01.7
176.03138 -27.90575 galactic Tau Second-epoch detections are separated by 0.4" 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.742 Edisona 0 1 1 14.5 -0 0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:59:31.69 +15:00:01.7: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:59:31.69 +15:00:01.7: 16.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 19.3738* 03 59 31.69 +15 00 01.7 14.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8738,14.29,0.05,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 20260919.3738 14.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 19.3738 2461302.8738 14.64 03:57:18.99 +11:56:52.4
178.21268 -30.35070 galactic Tau Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.655 Briseis 0 1 1 14.8 -0 -0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:57:18.99 +11:56:52.4: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:57:18.99 +11:56:52.4: 16.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 19.3738* 03 57 18.99 +11 56 52.4 14.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8738,14.64,0.05,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 20260919.3738 14.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 19.3738 2461302.8738 15.21 03:20:22.56 +17:00:41.0
166.53492 -32.96808 galactic Ari 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.1424 Sundmania -1 1 2 15.2 0 0
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:20:22.56 +17:00:41.0: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:20:22.56 +17:00:41.0: 16.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 19.3738* 03 20 22.56 +17 00 41.0 15.2 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461302.8738,15.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260919.3738 15.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
First image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Last image: 2461302.87418778 19.09.2026 08:58:39.824 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.43
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): 7792
Objects passed selection criteria: 7785
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 7355.75
Average stars matched: 7170.5 (97.4816 %)
Memory usage VmPeak: 233652 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Sep 19 04:00:33 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
First image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Last image: 2461302.87418778 19.09.2026 08:58:39.824 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 68
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.14
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: 19 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): 48333
Objects passed selection criteria: 48196
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 45804
Average stars matched: 44198 (96.4938 %)
Memory usage VmPeak: 267440 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Sep 19 04:01:33 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/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.cat to cache
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461302.87334199
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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits exists and is non-empty
wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits exists and is non-empty
wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (1st reference image)
verification OK: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:20.383 +13:59:53.59 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits (1st new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:38.445 +14:00:57.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:38.445 +14:00:57.00
Angular distance between the image centers 0.0751 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits (2nd new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:39.633 +14:00:15.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:39.633 +14:00:15.61
Angular distance between the image centers 0.0781 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 03:33:38.445 +14:00:57.00
Second-epoch second image center 03:33:39.633 +14:00:15.61
Angular distance between the image centers 0.01246 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/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits &> /tmp/tmp.HGOWyJ53OF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits &> /tmp/tmp.oplhXuqxVo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits &> /tmp/tmp.yi6Q1pX2Y1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits &> /tmp/tmp.nx24k3p0Pz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
The reference image (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits) and catalog (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat) found
'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat' -> 'wcsmag.cat'
Read 7716 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6428 deg, Dec +8.6205 to +19.2872 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 45.0636 to 61.6428 deg, Dec 8.6205 to 19.2872 deg
Loaded 4361 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): 3534 out of 3742 total matches.
Matched with Tycho-2 3742 out of 7716 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.950750
a=0.000000 b=1.000000 c=22.950750
From vast_summary.log: estimated ref. image limiting mag.: -7.43
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7716 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6428 deg, Dec +8.6205 to +19.2872 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 45.0636 to 61.6428 deg, Dec 8.6205 to 19.2872 deg
Loaded 4361 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): 3534 out of 3742 total matches.
Matched with Tycho-2 3742 out of 7716 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (aperture=6.0)
Read 7722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0650 to 61.6427 deg, Dec +8.6182 to +19.2791 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 45.0650 to 61.6427 deg, Dec 8.6182 to 19.2791 deg
Loaded 4354 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): 3534 out of 3736 total matches.
Matched with Tycho-2 3736 out of 7722 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
2.0 pix Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
2.3 pix fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
2.3 pix fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Limiting magnitude estimates:
15.5 mag. Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
15.5 mag. Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
15.3 mag. fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
15.3 mag. fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
All-image limiting magnitude estimate: 15.3 (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.HGOWyJ53OF (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_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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=551, bad_region=0, passed=7716
Got 7716 stars (including 7157 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 7716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 493 to 548 (Dec 8.6 to 19.3)
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: 4895 matched stars entering correct_measured_positions(), 4895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 493 to 548 (Dec 8.6 to 19.3)
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: 4895 matched stars entering correct_measured_positions(), 7716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4895 stars left (next iteration limit 5384)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits N_match=4895 sigma_overall_arcsec=0.305 sigma_q1_arcsec=0.404 sigma_q2_arcsec=0.301 sigma_q3_arcsec=0.272 sigma_q4_arcsec=0.248 n_q1=1380 n_q2=1359 n_q3=1203 n_q4=953 worst_quadrant_to_overall_ratio=1.327
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.oplhXuqxVo (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_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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=536, bad_region=0, passed=7722
Got 7722 stars (including 7177 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 7722 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 4900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 7722 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
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 7722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 7722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4900 stars left (next iteration limit 5390)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits N_match=4900 sigma_overall_arcsec=0.307 sigma_q1_arcsec=0.403 sigma_q2_arcsec=0.295 sigma_q3_arcsec=0.260 sigma_q4_arcsec=0.260 n_q1=1378 n_q2=1355 n_q3=1207 n_q4=960 worst_quadrant_to_overall_ratio=1.311
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.yi6Q1pX2Y1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.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=432, bad_region=0, passed=7066
Got 7066 stars (including 6627 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat
util/solve_plate_with_UCAC5 got 7066 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
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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 4895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7066 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
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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4895 stars left (next iteration limit 5384)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4895 robust_rms=12.498 arcsec worst_quadrant_rms=13.462 arcsec
SIP_REFIT: SIP order 3 trial: matched=4895 robust_rms=0.430 arcsec worst_quadrant_rms=0.448 arcsec
SIP_REFIT: SIP order 5 trial: matched=4895 robust_rms=0.290 arcsec worst_quadrant_rms=0.305 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4895 robust_rms_before=1.095 arcsec robust_rms_before_corrected=0.302 arcsec robust_rms_after=0.290 arcsec worst_quadrant_rms_before=0.319 worst_quadrant_rms_after=0.305
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.319 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits N_match=4895 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.331 sigma_q2_arcsec=0.335 sigma_q3_arcsec=0.305 sigma_q4_arcsec=0.296 n_q1=987 n_q2=1176 n_q3=1394 n_q4=1338 worst_quadrant_to_overall_ratio=1.064
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits -region wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.nx24k3p0Pz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.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=445, bad_region=0, passed=7083
Got 7083 stars (including 6628 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat
util/solve_plate_with_UCAC5 got 7083 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
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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 4896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 7083 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
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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 7083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 7083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4896 stars left (next iteration limit 5385)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4896 robust_rms=12.548 arcsec worst_quadrant_rms=13.115 arcsec
SIP_REFIT: SIP order 3 trial: matched=4896 robust_rms=0.419 arcsec worst_quadrant_rms=0.439 arcsec
SIP_REFIT: SIP order 5 trial: matched=4896 robust_rms=0.278 arcsec worst_quadrant_rms=0.295 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4896 robust_rms_before=1.083 arcsec robust_rms_before_corrected=0.289 arcsec robust_rms_after=0.278 arcsec worst_quadrant_rms_before=0.308 worst_quadrant_rms_after=0.295
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.308 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits N_match=4896 sigma_overall_arcsec=0.301 sigma_q1_arcsec=0.301 sigma_q2_arcsec=0.322 sigma_q3_arcsec=0.299 sigma_q4_arcsec=0.289 n_q1=991 n_q2=1172 n_q3=1394 n_q4=1339 worst_quadrant_to_overall_ratio=1.068
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits -region wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits to local_wcs_cache/
'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits'
Saving the final (post-refit) wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits to local_wcs_cache/
'wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits'
Saving the final (post-refit) wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits to local_wcs_cache/
'wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits' -> 'local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits'
Saving the final (post-refit) wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits to local_wcs_cache/
'wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits' -> 'local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits sigma_overall=0.305 worst_q_ratio=1.327
ref2=Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits sigma_overall=0.307 worst_q_ratio=1.311
new1=fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits sigma_overall=0.315 worst_q_ratio=1.064
new2=fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits sigma_overall=0.301 worst_q_ratio=1.068
reference average sigma_overall=0.306 worst_q_ratio=1.319
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_astrometric_residuals.png (4895 matched stars from wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_astrometric_residuals.png (4900 matched stars from wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408_astrometric_residuals.png (4895 matched stars from wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409_astrometric_residuals.png (4896 matched stars from wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits'
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits'
Preparing the HTML report for the field Tau-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:27:41.59 +12:04:09.7: 12.55 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:10:54.86 +19:07:00.6: 12.39 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:27:41.59 +12:04:09.7: 12.57 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:10:54.86 +19:07:00.6: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter REJECTED candidate at 03:27:41.59 +12:04:09.7: ref_mag=12.56 +/- 0.01 new_mean_mag=12.4820 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter REJECTED candidate at 03:10:54.86 +19:07:00.6: ref_mag=12.38 +/- 0.01 new_mean_mag=12.2999 delta=0.09 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20485_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 20485_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 03:54:23.48 +16:01:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20543_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 20543_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 03:32:41.24 +09:22:42.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20565_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 20565_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20576_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 20576_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 03:23:05.51 +18:34:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20595_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 20595_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Tau-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.cat to cache
SExtractor catalog cache: saved Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Creating symlink local_wcs_cache/wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Checking 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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits exists and is non-empty
wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits exists and is non-empty
wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (1st reference image)
verification OK: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:20.383 +13:59:53.59 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits (1st new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:38.445 +14:00:57.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:38.445 +14:00:57.00
Angular distance between the image centers 0.0751 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits (2nd new image)
verification OK: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:39.633 +14:00:15.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:39.633 +14:00:15.61
Angular distance between the image centers 0.0781 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 03:33:38.445 +14:00:57.00
Second-epoch second image center 03:33:39.633 +14:00:15.61
Angular distance between the image centers 0.01246 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/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits &> /tmp/tmp.03kENNL5fu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits &> /tmp/tmp.Ro1tUjd0IA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits &> /tmp/tmp.XzeJwaDS6x
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits &> /tmp/tmp.QPlhAgL1lD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
Found non-empty wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
The reference image (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits) and catalog (wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat) found
'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat' -> 'wcsmag.cat'
Read 48584 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6458 deg, Dec +8.6191 to +19.2871 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 45.0636 to 61.6458 deg, Dec 8.6191 to 19.2871 deg
Loaded 4361 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): 3309 out of 3760 total matches.
Matched with Tycho-2 3760 out of 48584 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.830300
a=0.000000 b=1.000000 c=22.830300
From vast_summary.log: estimated ref. image limiting mag.: -7.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.69
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.69
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 48584 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6458 deg, Dec +8.6191 to +19.2871 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 45.0636 to 61.6458 deg, Dec 8.6191 to 19.2871 deg
Loaded 4361 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): 3309 out of 3760 total matches.
Matched with Tycho-2 3760 out of 48584 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (aperture=4.6)
Read 48560 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0650 to 61.6548 deg, Dec +8.6183 to +19.2794 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 45.0650 to 61.6548 deg, Dec 8.6183 to 19.2794 deg
Loaded 4358 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): 3320 out of 3753 total matches.
Matched with Tycho-2 3753 out of 48560 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -> calib.txt_param_ref_wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 62 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
1.9 pix Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
2.2 pix fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
2.2 pix fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Limiting magnitude estimates:
15.7 mag. Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
15.7 mag. Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
15.5 mag. fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
15.5 mag. fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.8 (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.03kENNL5fu (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_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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=2222, bad_region=4, passed=48568
Got 48568 stars (including 46270 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 48568 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 4898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 48568 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
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 48568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 48568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4898 stars left (next iteration limit 5387)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits N_match=4898 sigma_overall_arcsec=0.295 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.289 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.252 n_q1=1362 n_q2=1350 n_q3=1192 n_q4=994 worst_quadrant_to_overall_ratio=1.312
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Ro1tUjd0IA (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_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS-calibrated image found: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Checking if the catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS catalog name: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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=2192, bad_region=5, passed=48544
Got 48544 stars (including 46257 good ones) from the SExtractor catalog wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 48544 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 4898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 48544 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
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 48544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 48544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4899 stars left (next iteration limit 5387)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits N_match=4899 sigma_overall_arcsec=0.297 sigma_q1_arcsec=0.379 sigma_q2_arcsec=0.293 sigma_q3_arcsec=0.255 sigma_q4_arcsec=0.256 n_q1=1361 n_q2=1351 n_q3=1201 n_q4=986 worst_quadrant_to_overall_ratio=1.274
The image catalog is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -region wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.XzeJwaDS6x (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1725, bad_region=31, passed=43591
Got 43591 stars (including 41759 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat
util/solve_plate_with_UCAC5 got 43591 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
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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4901 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(), 43591 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
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 491 to 549 (Dec 8.3 to 19.5)
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: 4891 matched stars entering correct_measured_positions(), 43591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 43591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.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=12.518 arcsec worst_quadrant_rms=13.079 arcsec
SIP_REFIT: SIP order 3 trial: matched=4891 robust_rms=0.426 arcsec worst_quadrant_rms=0.435 arcsec
SIP_REFIT: SIP order 5 trial: matched=4891 robust_rms=0.283 arcsec worst_quadrant_rms=0.301 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4891 robust_rms_before=1.071 arcsec robust_rms_before_corrected=0.294 arcsec robust_rms_after=0.283 arcsec worst_quadrant_rms_before=0.319 worst_quadrant_rms_after=0.301
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.319 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits N_match=4891 sigma_overall_arcsec=0.311 sigma_q1_arcsec=0.317 sigma_q2_arcsec=0.348 sigma_q3_arcsec=0.305 sigma_q4_arcsec=0.295 n_q1=1027 n_q2=1164 n_q3=1363 n_q4=1337 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits -region wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.QPlhAgL1lD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Checking if the catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
WCS catalog name: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.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=10, blended=1735, bad_region=36, passed=43605
Got 43605 stars (including 41760 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat
util/solve_plate_with_UCAC5 got 43605 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
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 491 to 549 (Dec 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4901 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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 43605 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
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 491 to 549 (Dec 8.3 to 19.5)
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: 4890 matched stars entering correct_measured_positions(), 43605 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 43605 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4890 stars left (next iteration limit 5379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.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=4890 robust_rms=12.349 arcsec worst_quadrant_rms=13.222 arcsec
SIP_REFIT: SIP order 3 trial: matched=4890 robust_rms=0.417 arcsec worst_quadrant_rms=0.432 arcsec
SIP_REFIT: SIP order 5 trial: matched=4890 robust_rms=0.271 arcsec worst_quadrant_rms=0.293 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4890 robust_rms_before=1.065 arcsec robust_rms_before_corrected=0.282 arcsec robust_rms_after=0.271 arcsec worst_quadrant_rms_before=0.309 worst_quadrant_rms_after=0.293
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.309 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits N_match=4890 sigma_overall_arcsec=0.295 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.324 sigma_q3_arcsec=0.283 sigma_q4_arcsec=0.283 n_q1=1024 n_q2=1154 n_q3=1383 n_q4=1329 worst_quadrant_to_overall_ratio=1.100
The image catalog is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits -region wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-57-26_20.00sec_0.00C_LIGHTs_0408.fits
Saving fully-calibrated image wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-19_CI_Tau-05-Q1b1x1_035914_TTUQ1b1x1_2328582_FFUJA1tp/wcs_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409.fits
Preparing the HTML report for the field Tau-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:33:04.07 +18:55:13.2: 14.64 +/- 0.09 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:23:44.49 +17:35:45.4: 15.29 +/- 0.16 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:52.15 +10:46:43.4: 14.41 +/- 0.08 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:45:33.55 +12:52:25.5: 14.39 +/- 0.07 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:10:19.39 +11:34:31.3: 14.85 +/- 0.11 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:56:24.18 +10:19:37.6: 14.73 +/- 0.11 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:14:45.01 +14:04:33.1: 13.52 +/- 0.03 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:10:59.15 +14:33:27.1: 14.62 +/- 0.08 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:14:21.31 +10:20:52.5: 12.86 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:45:33.55 +12:52:25.5: 14.35 +/- 0.07 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:10:59.15 +14:33:27.1: 14.58 +/- 0.09 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:10:19.39 +11:34:31.3: 14.78 +/- 0.11 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:56:24.18 +10:19:37.6: 14.72 +/- 0.11 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:33:04.07 +18:55:13.2: 14.78 +/- 0.10 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:52.15 +10:46:43.4: 14.52 +/- 0.09 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:23:44.49 +17:35:45.4: 15.05 +/- 0.13 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:14:45.01 +14:04:33.1: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.06
Forced photometry reference-image weighted average: 14.37 +/- 0.05
Forced photometry reference-image weighted average: 14.72 +/- 0.08
Forced photometry reference-image weighted average: 14.82 +/- 0.08
Forced photometry filter REJECTED candidate at 03:10:59.15 +14:33:27.1: ref_mag=14.60 +/- 0.06 new_mean_mag=14.7446 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:45:33.55 +12:52:25.5: ref_mag=14.37 +/- 0.05 new_mean_mag=14.4679 delta=-0.10 (need > 0.90)
Forced photometry reference-image weighted average: 14.70 +/- 0.07
Forced photometry filter REJECTED candidate at 03:10:19.39 +11:34:31.3: ref_mag=14.82 +/- 0.08 new_mean_mag=14.9289 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:56:24.18 +10:19:37.6: ref_mag=14.72 +/- 0.08 new_mean_mag=14.9325 delta=-0.21 (need > 0.90)
Forced photometry reference-image weighted average: 15.15 +/- 0.10
Forced photometry reference-image weighted average: 14.46 +/- 0.06
Forced photometry filter REJECTED candidate at 03:33:04.07 +18:55:13.2: ref_mag=14.70 +/- 0.07 new_mean_mag=14.9137 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:23:44.49 +17:35:45.4: ref_mag=15.15 +/- 0.10 new_mean_mag=15.0765 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Forced photometry filter REJECTED candidate at 03:37:52.15 +10:46:43.4: ref_mag=14.46 +/- 0.06 new_mean_mag=14.6022 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:14:45.01 +14:04:33.1: ref_mag=13.49 +/- 0.02 new_mean_mag=13.7348 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:21:09.94 +17:40:36.2: 12.47 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:14:21.31 +10:20:52.5: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter REJECTED candidate at 03:14:21.31 +10:20:52.5: ref_mag=12.84 +/- 0.01 new_mean_mag=13.0413 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:21:09.94 +17:40:36.2: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter REJECTED candidate at 03:21:09.94 +17:40:36.2: ref_mag=12.48 +/- 0.01 new_mean_mag=12.6544 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:18:27.84 +10:16:18.3: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:02:28.29 +13:27:56.5: 12.68 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:30:41.74 +18:27:58.0: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 04:05:03.15 +17:55:18.2: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:06:07.85 +16:20:01.8: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:09:30.59 +13:36:17.8: 12.26 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:55:13.96 +16:23:56.2: 16.08 +/- 0.35 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:10:07.71 +14:50:47.5: 14.16 +/- 0.06 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 04:05:03.15 +17:55:18.2: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:02:28.29 +13:27:56.5: 12.62 +/- 0.02 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:18:27.84 +10:16:18.3: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:30:41.74 +18:27:58.0: 16.18 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter REJECTED candidate at 03:02:28.29 +13:27:56.5: ref_mag=12.65 +/- 0.01 new_mean_mag=12.8214 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:06:07.85 +16:20:01.8: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:09:30.59 +13:36:17.8: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter REJECTED candidate at 03:09:30.59 +13:36:17.8: ref_mag=12.23 +/- 0.01 new_mean_mag=12.4202 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:50:22.02 +17:07:13.6: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:55:13.96 +16:23:56.2: 16.09 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 16.08 +/- 0.35
Forced photometry filter KEPT candidate at 03:55:13.96 +16:23:56.2: ref_mag=16.08 +/- 0.35 new_mean_mag=13.7797 delta=2.30 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:10:07.71 +14:50:47.5: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Forced photometry filter REJECTED candidate at 03:10:07.71 +14:50:47.5: ref_mag=14.10 +/- 0.04 new_mean_mag=14.1529 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:23:30.54 +17:10:26.4: 14.38 +/- 0.08 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:50:22.02 +17:07:13.6: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:59:31.69 +15:00:01.7: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:02:09.60 +12:02:07.5: 15.00 +/- 0.15 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:23:30.54 +17:10:26.4: 14.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.05
Forced photometry filter REJECTED candidate at 03:23:30.54 +17:10:26.4: ref_mag=14.37 +/- 0.05 new_mean_mag=14.3877 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:59:31.69 +15:00:01.7: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:20:24.33 +14:19:16.0: 14.40 +/- 0.07 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:02:09.60 +12:02:07.5: 14.76 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.09
Forced photometry filter REJECTED candidate at 03:02:09.60 +12:02:07.5: ref_mag=14.85 +/- 0.09 new_mean_mag=14.5686 delta=0.28 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:20:24.33 +14:19:16.0: 14.47 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.05
Forced photometry filter REJECTED candidate at 03:20:24.33 +14:19:16.0: ref_mag=14.43 +/- 0.05 new_mean_mag=14.5260 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:34:18.80 +10:38:18.1: 14.56 +/- 0.08 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:20:36.58 +14:40:20.7: 14.87 +/- 0.11 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:34:18.80 +10:38:18.1: 14.47 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.06
Forced photometry filter REJECTED candidate at 03:34:18.80 +10:38:18.1: ref_mag=14.51 +/- 0.06 new_mean_mag=14.6058 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:20:36.58 +14:40:20.7: 14.58 +/- 0.08 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:05:22.74 +14:15:38.5: 14.94 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.06
Forced photometry filter REJECTED candidate at 03:20:36.58 +14:40:20.7: ref_mag=14.69 +/- 0.06 new_mean_mag=14.7706 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:05:22.74 +14:15:38.5: 15.31 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.11
Forced photometry filter REJECTED candidate at 03:05:22.74 +14:15:38.5: ref_mag=15.05 +/- 0.11 new_mean_mag=14.8885 delta=0.16 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:03:31.14 +14:12:37.0: 14.94 +/- 0.14 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 04:02:25.91 +18:13:51.6: 14.92 +/- 0.14 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:03:31.14 +14:12:37.0: 15.05 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.10
Forced photometry filter REJECTED candidate at 03:03:31.14 +14:12:37.0: ref_mag=14.99 +/- 0.10 new_mean_mag=14.9447 delta=0.05 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 04:02:25.91 +18:13:51.6: 15.19 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.12
Forced photometry filter REJECTED candidate at 04:02:25.91 +18:13:51.6: ref_mag=15.02 +/- 0.12 new_mean_mag=14.6400 delta=0.38 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:57:18.99 +11:56:52.4: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:57:18.99 +11:56:52.4: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:09:00.22 +15:36:42.7: 15.14 +/- 0.15 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:08:52.11 +14:15:28.8: 14.94 +/- 0.13 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:09:00.22 +15:36:42.7: 15.34 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.22 +/- 0.11
Forced photometry filter REJECTED candidate at 03:09:00.22 +15:36:42.7: ref_mag=15.22 +/- 0.11 new_mean_mag=14.9240 delta=0.30 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:08:52.11 +14:15:28.8: 14.79 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.09
Forced photometry filter REJECTED candidate at 03:08:52.11 +14:15:28.8: ref_mag=14.85 +/- 0.09 new_mean_mag=14.8057 delta=0.05 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:06:50.01 +12:24:38.0: 15.07 +/- 0.15 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:05:42.57 +12:53:46.2: 14.53 +/- 0.09 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:06:50.01 +12:24:38.0: 15.21 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.11
Forced photometry filter REJECTED candidate at 03:06:50.01 +12:24:38.0: ref_mag=15.13 +/- 0.11 new_mean_mag=15.0263 delta=0.11 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:05:42.57 +12:53:46.2: 14.72 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.07
Forced photometry filter REJECTED candidate at 03:05:42.57 +12:53:46.2: ref_mag=14.61 +/- 0.07 new_mean_mag=14.8188 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:06:48.25 +10:44:49.3: 15.76 +/- 0.29 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:25:16.35 +09:31:26.0: 15.24 +/- 0.16 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:06:48.25 +10:44:49.3: 15.50 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.59 +/- 0.18
Forced photometry filter REJECTED candidate at 03:06:48.25 +10:44:49.3: ref_mag=15.59 +/- 0.18 new_mean_mag=15.0354 delta=0.56 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:25:16.35 +09:31:26.0: 15.35 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.29 +/- 0.12
Forced photometry filter REJECTED candidate at 03:25:16.35 +09:31:26.0: ref_mag=15.29 +/- 0.12 new_mean_mag=15.0089 delta=0.28 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:08:36.59 +09:21:14.0: 15.22 +/- 0.18 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:10:38.85 +11:40:44.3: 15.58 +/- 0.21 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:08:36.59 +09:21:14.0: 15.07 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.12
Forced photometry filter REJECTED candidate at 03:08:36.59 +09:21:14.0: ref_mag=15.13 +/- 0.12 new_mean_mag=15.0440 delta=0.09 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:10:38.85 +11:40:44.3: 15.49 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.53 +/- 0.15
Forced photometry filter REJECTED candidate at 03:10:38.85 +11:40:44.3: ref_mag=15.53 +/- 0.15 new_mean_mag=15.0453 delta=0.48 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:10:07.29 +11:45:21.9: 15.24 +/- 0.16 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:09:37.59 +13:05:00.7: 15.16 +/- 0.15 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:10:07.29 +11:45:21.9: 15.15 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.11
Forced photometry filter REJECTED candidate at 03:10:07.29 +11:45:21.9: ref_mag=15.19 +/- 0.11 new_mean_mag=15.0495 delta=0.14 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:09:37.59 +13:05:00.7: 15.37 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.12
Forced photometry filter REJECTED candidate at 03:09:37.59 +13:05:00.7: ref_mag=15.24 +/- 0.12 new_mean_mag=14.9963 delta=0.25 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:18:30.76 +09:56:31.7: 15.05 +/- 0.14 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:09:26.74 +12:21:47.3: 15.31 +/- 0.17 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:18:30.76 +09:56:31.7: 15.37 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.11
Forced photometry filter REJECTED candidate at 03:18:30.76 +09:56:31.7: ref_mag=15.16 +/- 0.11 new_mean_mag=15.0890 delta=0.07 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:09:26.74 +12:21:47.3: 15.34 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.32 +/- 0.13
Forced photometry filter REJECTED candidate at 03:09:26.74 +12:21:47.3: ref_mag=15.32 +/- 0.13 new_mean_mag=15.1516 delta=0.17 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:13:36.36 +14:47:43.1: 15.40 +/- 0.21 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:31:49.45 +15:08:03.6: 15.03 +/- 0.12 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:13:36.36 +14:47:43.1: 15.51 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.45 +/- 0.15
Forced photometry filter REJECTED candidate at 03:13:36.36 +14:47:43.1: ref_mag=15.45 +/- 0.15 new_mean_mag=15.0659 delta=0.38 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:31:49.45 +15:08:03.6: 14.93 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.08
Forced photometry filter REJECTED candidate at 03:31:49.45 +15:08:03.6: ref_mag=14.98 +/- 0.08 new_mean_mag=14.7990 delta=0.18 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 04:02:46.64 +15:37:46.6: 15.23 +/- 0.18 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:05:51.76 +14:26:19.5: 15.22 +/- 0.17 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:06:19.58 +15:43:01.8: 15.18 +/- 0.15 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:20:42.69 +18:39:58.0: 15.52 +/- 0.21 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 04:02:46.64 +15:37:46.6: 15.67 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.37 +/- 0.15
Forced photometry filter REJECTED candidate at 04:02:46.64 +15:37:46.6: ref_mag=15.37 +/- 0.15 new_mean_mag=14.9713 delta=0.39 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:05:51.76 +14:26:19.5: 15.26 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.12
Forced photometry filter REJECTED candidate at 03:05:51.76 +14:26:19.5: ref_mag=15.24 +/- 0.12 new_mean_mag=15.0068 delta=0.23 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:06:19.58 +15:43:01.8: 15.32 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.12
Forced photometry filter REJECTED candidate at 03:06:19.58 +15:43:01.8: ref_mag=15.23 +/- 0.12 new_mean_mag=15.0546 delta=0.18 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:20:42.69 +18:39:58.0: 16.15 +/- 0.36 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:22:56.19 +17:27:13.6: 15.50 +/- 0.20 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:11:59.37 +13:22:10.7: 15.31 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.67 +/- 0.18
Forced photometry filter REJECTED candidate at 03:20:42.69 +18:39:58.0: ref_mag=15.67 +/- 0.18 new_mean_mag=15.0958 delta=0.58 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:18:37.47 +12:34:55.8: 15.33 +/- 0.16 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:20:22.56 +17:00:41.0: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:11:59.37 +13:22:10.7: 15.40 +/- 0.19 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:22:56.19 +17:27:13.6: 15.31 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.35 +/- 0.13
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:53:39.38 +18:02:02.0: 14.97 +/- 0.13 detection
Forced photometry reference-image weighted average: 15.39 +/- 0.13
Forced photometry filter REJECTED candidate at 03:11:59.37 +13:22:10.7: ref_mag=15.35 +/- 0.13 new_mean_mag=15.1012 delta=0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:22:56.19 +17:27:13.6: ref_mag=15.39 +/- 0.13 new_mean_mag=15.0962 delta=0.29 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:42:54.19 +15:02:02.9: 15.13 +/- 0.13 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:18:37.47 +12:34:55.8: 15.67 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.45 +/- 0.13
Forced photometry filter REJECTED candidate at 03:18:37.47 +12:34:55.8: ref_mag=15.45 +/- 0.13 new_mean_mag=15.1728 delta=0.28 (need > 0.90)
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:20:22.56 +17:00:41.0: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:53:39.38 +18:02:02.0: 15.12 +/- 0.16 detection
Forced photometry on wcs_Tau-05-Q1b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:42:54.19 +15:02:02.9: 15.25 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.10
Forced photometry filter REJECTED candidate at 03:53:39.38 +18:02:02.0: ref_mag=15.04 +/- 0.10 new_mean_mag=14.9166 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 15.18 +/- 0.10
Forced photometry filter REJECTED candidate at 03:42:54.19 +15:02:02.9: ref_mag=15.18 +/- 0.10 new_mean_mag=15.0791 delta=0.10 (need > 0.90)
Adding exclusion_list_local.txt__out53852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54893.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 53533_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53533_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53536_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53536_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53538_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53538_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53539_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53539_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53540_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53540_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53548_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53548_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53553_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53553_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 03:02:03.85 +13:52:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53555_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53555_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53557_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53557_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 04:06:06.10 +16:08:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53560_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53560_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53563_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53563_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53565_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53565_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 03:32:32.68 +15:13:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53566_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53566_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53567_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53567_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53822_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53822_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 53852_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
Preparing report for the candidate 53852_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
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Considering the candidate 53914_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53914_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 03:54:47.28 +09:11:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53955_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
Preparing report for the candidate 53955_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
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Considering the candidate 53991_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
Preparing report for the candidate 53991_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
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Considering the candidate 53995_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 53995_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 03:36:02.15 +16:29:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54079_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
Preparing report for the candidate 54079_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
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Considering the candidate 54144_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
Preparing report for the candidate 54144_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
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Considering the candidate 54230_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54230_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 03:07:55.09 +16:03:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54246_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54246_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54363_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54363_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 03:54:00.20 +15:36:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54367_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
Preparing report for the candidate 54367_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
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Considering the candidate 54387_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54387_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54433_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
Preparing report for the candidate 54433_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
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Considering the candidate 54480_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54480_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54492_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54492_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54585_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54585_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54596_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54596_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54621_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54621_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54623_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54623_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54653_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54653_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54662_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
Preparing report for the candidate 54662_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
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Considering the candidate 54666_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54666_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54667_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54667_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54724_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54724_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54733_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54733_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54750_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54750_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54759_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54759_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54767_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54767_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54768_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54768_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54769_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54769_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54775_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54775_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54792_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54792_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54796_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54796_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54814_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54814_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54817_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54817_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54825_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54825_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54827_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54827_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54831_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54831_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54834_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54834_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54842_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54842_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54867_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54867_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54885_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54885_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54893_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
Preparing report for the candidate 54893_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
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Considering the candidate 54923_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54923_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 54933_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 54933_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
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Considering the candidate 17153_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 17153_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
**** FOUND 03:54:23.47 +16:01:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03893_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409
The candidate 03893_fd_Tau-05-Q1b1x1_2026-09-19_03-58-39_20.00sec_-0.00C_LIGHTs_0409 did not pass the final checks
