This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf
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 09.4474 2461292.9474 12.41 03:37:11.51 +21:03:14.4
166.96941 -27.31247 galactic Tau Second-epoch detections are separated by 0.4" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.64 Angelina -1 -1 2 12.5 -0 0
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:37:11.51 +21:03:14.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:37:11.51 +21:03:14.4: 16.11 +/- 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 09.4474* 03 37 11.51 +21 03 14.4 12.4 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,2461292.9474,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4474 12.41CV 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 09.4474 2461292.9474 12.88 03:26:56.89 +18:41:11.5
166.66755 -30.67917 galactic Tau Second-epoch detections are separated by 0.7" and 8.2 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 12.9 -0 0
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:26:56.89 +18:41:11.5: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:26:56.89 +18:41:11.5: 16.15 +/- 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 09.4474* 03 26 56.89 +18 41 11.5 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,2461292.9474,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4474 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 09.4474 2461292.9474 13.46 03:59:28.10 +17:48:09.5
173.72375 -26.00257 galactic Tau Second-epoch detections are separated by 0.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.62 Erato 0 -0 0 13.7 -0 0
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:59:28.10 +17:48:09.5: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:59:28.10 +17:48:09.5: 16.11 +/- 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 09.4474* 03 59 28.10 +17 48 09.5 13.5 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,2461292.9474,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4474 13.46CV 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 09.4474 2461292.9474 14.48 03:26:46.41 +22:44:39.1
163.66056 -27.58548 galactic Ari Second-epoch detections are separated by 0.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.830 Petropolitana -1 -0 1 14.6 0 0
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:26:46.41 +22:44:39.1: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:26:46.41 +22:44:39.1: 16.33 +/- 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 09.4474* 03 26 46.41 +22 44 39.1 14.5 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,2461292.9474,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4474 14.48CV 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 09.4474 2461292.9474 14.44 03:26:34.37 +19:12:22.6
166.19831 -30.34067 galactic Tau Second-epoch detections are separated by 0.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.586 Thekla -1 -1 1 14.8 -0 0
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:26:34.37 +19:12:22.6: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:26:34.37 +19:12:22.6: 16.22 +/- 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 09.4474* 03 26 34.37 +19 12 22.6 14.4 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,2461292.9474,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4474 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4474 2461292.9474 14.74 03:37:51.71 +26:01:42.0
163.50028 -23.44591 galactic Tau Second-epoch detections are separated by 4.6" 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.613 Ginevra -2 -1 2 14.9 -0 0
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:37:51.71 +26:01:42.0: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:37:51.71 +26:01:42.0: 16.23 +/- 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 09.4474* 03 37 51.71 +26 01 42.0 14.7 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,2461292.9474,14.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4474 14.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 09.4474 2461292.9474 14.96 03:45:30.91 +20:57:22.9
168.65177 -26.07793 galactic Tau Second-epoch detections are separated by 1.0" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.859 Bouzareah 0 -0 0 14.9 0 0
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:45:30.91 +20:57:22.9: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:45:30.91 +20:57:22.9: 16.29 +/- 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 09.4474* 03 45 30.91 +20 57 22.9 15.0 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,2461292.9474,14.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4474 14.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
First image: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Last image: 2461292.94785816 09.09.2026 10:44:44.945 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 5 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): 10559
Objects passed selection criteria: 10529
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 8405.75
Average stars matched: 7739.25 (92.0709 %)
Memory usage VmPeak: 236100 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Sep 9 05:59:02 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
First image: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Last image: 2461292.94785816 09.09.2026 10:44:44.945 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 81
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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: 28 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): 66709
Objects passed selection criteria: 66483
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 54530.8
Average stars matched: 50017.5 (91.7235 %)
Memory usage VmPeak: 282972 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Sep 9 06:00:19 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat to cache
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461292.94694543
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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits exists and is non-empty
wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits exists and is non-empty
wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits exists and is non-empty
wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (1st reference image)
verification OK: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Image size: 941.6'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: 03:41:33.276 +21:59:52.28 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-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits (1st new image)
verification OK: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:41:31.615 +22:00:00.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:41:33.276 +21:59:52.28
Second-epoch image center 03:41:31.615 +22:00:00.30
Angular distance between the image centers 0.0068 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits (2nd new image)
verification OK: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:41:30.005 +22:00:42.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:41:33.276 +21:59:52.28
Second-epoch image center 03:41:30.005 +22:00:42.30
Angular distance between the image centers 0.0188 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 03:41:31.615 +22:00:00.30
Second-epoch second image center 03:41:30.005 +22:00:42.30
Angular distance between the image centers 0.01322 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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits &> /tmp/tmp.cBt5GKC4g4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits &> /tmp/tmp.kVi4EcsWTM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits &> /tmp/tmp.zbCqtXkuMn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits &> /tmp/tmp.gRnmt1lrOU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
The reference image (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits) and catalog (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat) found
'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat' -> 'wcsmag.cat'
Read 11324 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6706 to 64.2537 deg, Dec +16.5354 to +27.2942 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 46.6706 to 64.2537 deg, Dec 16.5354 to 27.2942 deg
Loaded 6127 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): 4779 out of 5136 total matches.
Matched with Tycho-2 5136 out of 11324 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.939900
a=0.000000 b=1.000000 c=22.939900
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11324 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6706 to 64.2537 deg, Dec +16.5354 to +27.2942 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 46.6706 to 64.2537 deg, Dec 16.5354 to 27.2942 deg
Loaded 6127 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): 4779 out of 5136 total matches.
Matched with Tycho-2 5136 out of 11324 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Forced-photometry filter: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits -> calib.txt_param_ref_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (aperture=6.0)
Read 11315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6502 to 64.2538 deg, Dec +16.5175 to +27.2929 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 46.6502 to 64.2538 deg, Dec 16.5175 to 27.2929 deg
Loaded 6135 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): 4761 out of 5130 total matches.
Matched with Tycho-2 5130 out of 11315 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Forced-photometry filter: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits -> calib.txt_param_ref_wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
2.0 pix Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
2.2 pix fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
2.2 pix fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Limiting magnitude estimates:
15.4 mag. Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
15.4 mag. Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
15.2 mag. fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
15.2 mag. fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
All-image limiting magnitude estimate: 15.2 (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.cBt5GKC4g4 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=882, bad_region=2358, passed=11324
Got 11324 stars (including 8232 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
util/solve_plate_with_UCAC5 got 11324 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 4928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 9434 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 9434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 9434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4928 stars left (next iteration limit 5420)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits N_match=4928 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.265 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.233 n_q1=1932 n_q2=884 n_q3=1338 n_q4=774 worst_quadrant_to_overall_ratio=1.268
The image catalog is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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.kVi4EcsWTM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=893, bad_region=2356, passed=11315
Got 11315 stars (including 8229 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat
util/solve_plate_with_UCAC5 got 11315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 4927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 9430 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 9430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 9430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4927 stars left (next iteration limit 5419)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits N_match=4927 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.419 sigma_q2_arcsec=0.296 sigma_q3_arcsec=0.287 sigma_q4_arcsec=0.244 n_q1=1928 n_q2=891 n_q3=1332 n_q4=776 worst_quadrant_to_overall_ratio=1.303
The image catalog is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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.zbCqtXkuMn (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_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=690, bad_region=2244, passed=10167
Got 10167 stars (including 7359 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat
util/solve_plate_with_UCAC5 got 10167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4924 matched stars entering correct_measured_positions(), 4924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4924 matched stars entering correct_measured_positions(), 8465 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 8465 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 8465 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4925 stars left (next iteration limit 5416)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4925 robust_rms=6.891 arcsec worst_quadrant_rms=8.113 arcsec
SIP_REFIT: SIP order 3 trial: matched=4925 robust_rms=0.506 arcsec worst_quadrant_rms=0.665 arcsec
SIP_REFIT: SIP order 5 trial: matched=4925 robust_rms=0.372 arcsec worst_quadrant_rms=0.428 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4925 robust_rms_before=1.173 arcsec robust_rms_before_corrected=0.381 arcsec robust_rms_after=0.372 arcsec worst_quadrant_rms_before=0.428 worst_quadrant_rms_after=0.428
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.428 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits N_match=4925 sigma_overall_arcsec=0.400 sigma_q1_arcsec=0.331 sigma_q2_arcsec=0.422 sigma_q3_arcsec=0.466 sigma_q4_arcsec=0.397 n_q1=1367 n_q2=847 n_q3=1456 n_q4=1255 worst_quadrant_to_overall_ratio=1.166
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits -region wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.gRnmt1lrOU (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_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.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_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=734, bad_region=2222, passed=10184
Got 10184 stars (including 7366 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat
util/solve_plate_with_UCAC5 got 10184 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4924 matched stars entering correct_measured_positions(), 4924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4924 matched stars entering correct_measured_positions(), 8485 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4926 matched stars entering correct_measured_positions(), 8485 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4926 matched stars entering correct_measured_positions(), 8485 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4926 stars left (next iteration limit 5416)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4926 robust_rms=6.966 arcsec worst_quadrant_rms=7.984 arcsec
SIP_REFIT: SIP order 3 trial: matched=4926 robust_rms=0.554 arcsec worst_quadrant_rms=0.691 arcsec
SIP_REFIT: SIP order 5 trial: matched=4926 robust_rms=0.410 arcsec worst_quadrant_rms=0.465 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4926 robust_rms_before=1.170 arcsec robust_rms_before_corrected=0.415 arcsec robust_rms_after=0.410 arcsec worst_quadrant_rms_before=0.457 worst_quadrant_rms_after=0.465
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.457 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits N_match=4926 sigma_overall_arcsec=0.432 sigma_q1_arcsec=0.358 sigma_q2_arcsec=0.484 sigma_q3_arcsec=0.496 sigma_q4_arcsec=0.426 n_q1=1368 n_q2=852 n_q3=1450 n_q4=1256 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits -region wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits to local_wcs_cache/
'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits' -> 'local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits'
Saving the final (post-refit) wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits to local_wcs_cache/
'wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits' -> 'local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits'
Saving the final (post-refit) wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits to local_wcs_cache/
'wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits' -> 'local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits'
Saving the final (post-refit) wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits to local_wcs_cache/
'wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits' -> 'local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits sigma_overall=0.300 worst_q_ratio=1.268
ref2=Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits sigma_overall=0.322 worst_q_ratio=1.303
new1=fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits sigma_overall=0.400 worst_q_ratio=1.166
new2=fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits sigma_overall=0.432 worst_q_ratio=1.149
reference average sigma_overall=0.311 worst_q_ratio=1.2855
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145_astrometric_residuals.png (4928 matched stars from wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146_astrometric_residuals.png (4927 matched stars from wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367_astrometric_residuals.png (4925 matched stars from wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368_astrometric_residuals.png (4926 matched stars from wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits'
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits'
Preparing the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:37:11.51 +21:03:14.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:51:13.12 +22:06:36.9: 12.46 +/- 0.01 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:37:11.51 +21:03:14.4: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:51:13.12 +22:06:36.9: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter REJECTED candidate at 03:51:13.12 +22:06:36.9: ref_mag=12.46 +/- 0.01 new_mean_mag=12.2910 delta=0.17 (need > 0.90)
Adding exclusion_list_local.txt__out22120.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 21933_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 21933_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 22120_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
Preparing report for the candidate 22120_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:37:11.51 +21:03:14.4
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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat to cache
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Creating symlink local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits exists and is non-empty
wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits exists and is non-empty
wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits exists and is non-empty
wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (1st reference image)
verification OK: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Image size: 941.6'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: 03:41:33.276 +21:59:52.28 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-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits (1st new image)
verification OK: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:41:31.615 +22:00:00.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:41:33.276 +21:59:52.28
Second-epoch image center 03:41:31.615 +22:00:00.30
Angular distance between the image centers 0.0068 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits (2nd new image)
verification OK: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:41:30.005 +22:00:42.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:41:33.276 +21:59:52.28
Second-epoch image center 03:41:30.005 +22:00:42.30
Angular distance between the image centers 0.0188 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 03:41:31.615 +22:00:00.30
Second-epoch second image center 03:41:30.005 +22:00:42.30
Angular distance between the image centers 0.01322 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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits &> /tmp/tmp.oDoCOIjCgc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits &> /tmp/tmp.BYWZdGJ0Jn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits &> /tmp/tmp.jBOJZntjiX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits &> /tmp/tmp.klHSEUIYWI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
The reference image (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits) and catalog (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat) found
'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat' -> 'wcsmag.cat'
Read 71179 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6551 to 64.2537 deg, Dec +16.4774 to +27.2939 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 46.6551 to 64.2537 deg, Dec 16.4774 to 27.2939 deg
Loaded 6152 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): 4354 out of 5188 total matches.
Matched with Tycho-2 5188 out of 71179 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.815850
a=0.000000 b=1.000000 c=22.815850
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 71179 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6551 to 64.2537 deg, Dec +16.4774 to +27.2939 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 46.6551 to 64.2537 deg, Dec 16.4774 to 27.2939 deg
Loaded 6152 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): 4354 out of 5188 total matches.
Matched with Tycho-2 5188 out of 71179 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Forced-photometry filter: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits -> calib.txt_param_ref_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (aperture=4.6)
Read 71492 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6502 to 64.2538 deg, Dec +16.4673 to +27.2929 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 46.6502 to 64.2538 deg, Dec 16.4673 to 27.2929 deg
Loaded 6157 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): 4359 out of 5185 total matches.
Matched with Tycho-2 5185 out of 71492 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Forced-photometry filter: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits -> calib.txt_param_ref_wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits (aperture=4.5)
____ 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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
1.9 pix Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
2.1 pix fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
2.0 pix fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Limiting magnitude estimates:
15.6 mag. Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
15.6 mag. Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
15.4 mag. fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
15.4 mag. fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
All-image limiting magnitude estimate: 15.4 (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.oDoCOIjCgc (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=4312, bad_region=11991, passed=71155
Got 71155 stars (including 55407 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
util/solve_plate_with_UCAC5 got 71155 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4935 matched stars entering correct_measured_positions(), 4935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4935 matched stars entering correct_measured_positions(), 61742 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4935 matched stars entering correct_measured_positions(), 61742 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4935 matched stars entering correct_measured_positions(), 61742 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4935 stars left (next iteration limit 5428)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits N_match=4935 sigma_overall_arcsec=0.291 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.270 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.232 n_q1=1854 n_q2=887 n_q3=1405 n_q4=789 worst_quadrant_to_overall_ratio=1.237
The image catalog is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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.BYWZdGJ0Jn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=4374, bad_region=12029, passed=71479
Got 71479 stars (including 55644 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat
util/solve_plate_with_UCAC5 got 71479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 4930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 62079 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 62079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 62079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4930 stars left (next iteration limit 5423)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits N_match=4930 sigma_overall_arcsec=0.306 sigma_q1_arcsec=0.386 sigma_q2_arcsec=0.285 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.246 n_q1=1847 n_q2=888 n_q3=1401 n_q4=794 worst_quadrant_to_overall_ratio=1.261
The image catalog is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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.jBOJZntjiX (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_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=3535, bad_region=12601, passed=62884
Got 62884 stars (including 47403 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat
util/solve_plate_with_UCAC5 got 62884 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 4925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 53593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 53593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 53593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4925 stars left (next iteration limit 5417)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.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=4925 robust_rms=6.833 arcsec worst_quadrant_rms=7.967 arcsec
SIP_REFIT: SIP order 3 trial: matched=4925 robust_rms=0.491 arcsec worst_quadrant_rms=0.654 arcsec
SIP_REFIT: SIP order 5 trial: matched=4925 robust_rms=0.359 arcsec worst_quadrant_rms=0.414 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4925 robust_rms_before=1.147 arcsec robust_rms_before_corrected=0.366 arcsec robust_rms_after=0.359 arcsec worst_quadrant_rms_before=0.416 worst_quadrant_rms_after=0.414
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.416 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits N_match=4925 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.399 sigma_q3_arcsec=0.439 sigma_q4_arcsec=0.389 n_q1=1403 n_q2=909 n_q3=1426 n_q4=1187 worst_quadrant_to_overall_ratio=1.133
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits -region wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.klHSEUIYWI (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_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.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_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=3521, bad_region=12746, passed=63185
Got 63185 stars (including 47609 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat
util/solve_plate_with_UCAC5 got 63185 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 4926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 53784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 53784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 53784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4925 stars left (next iteration limit 5417)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.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=4925 robust_rms=6.919 arcsec worst_quadrant_rms=7.763 arcsec
SIP_REFIT: SIP order 3 trial: matched=4925 robust_rms=0.531 arcsec worst_quadrant_rms=0.673 arcsec
SIP_REFIT: SIP order 5 trial: matched=4925 robust_rms=0.394 arcsec worst_quadrant_rms=0.458 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4925 robust_rms_before=1.141 arcsec robust_rms_before_corrected=0.396 arcsec robust_rms_after=0.394 arcsec worst_quadrant_rms_before=0.449 worst_quadrant_rms_after=0.458
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.449 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits N_match=4925 sigma_overall_arcsec=0.414 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.436 sigma_q3_arcsec=0.480 sigma_q4_arcsec=0.407 n_q1=1408 n_q2=904 n_q3=1417 n_q4=1196 worst_quadrant_to_overall_ratio=1.161
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits -region wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.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-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-43-26_20.00sec_-0.00C_LIGHT_0367.fits
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.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_2026-09-09_CI_Tau-02-Q2b1x1_055649_TTUQ2b1x1_153812_L6MyOYtf/wcs_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368.fits
Preparing the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:53:42.07 +21:24:54.7: 14.55 +/- 0.07 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:23:57.21 +18:01:19.9: 14.59 +/- 0.09 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:22:43.63 +26:02:28.9: 14.63 +/- 0.09 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:59:28.44 +21:37:03.6: 15.22 +/- 0.14 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:27:30.81 +18:45:00.5: 15.66 +/- 0.22 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:58:01.61 +19:39:53.5: 14.82 +/- 0.11 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:35:10.67 +20:29:07.3: 14.52 +/- 0.07 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:30:09.23 +20:36:19.7: 14.57 +/- 0.08 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:50:36.21 +23:12:30.6: 15.29 +/- 0.15 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:33:51.13 +20:02:40.4: 14.19 +/- 0.05 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:22:43.63 +26:02:28.9: 14.56 +/- 0.09 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:59:28.44 +21:37:03.6: 15.06 +/- 0.13 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:58:01.61 +19:39:53.5: 14.70 +/- 0.09 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:30:09.23 +20:36:19.7: 14.67 +/- 0.09 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:23:57.21 +18:01:19.9: 14.68 +/- 0.09 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:50:36.21 +23:12:30.6: 15.15 +/- 0.13 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:27:30.81 +18:45:00.5: 15.47 +/- 0.18 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:35:10.67 +20:29:07.3: 14.56 +/- 0.07 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:33:51.13 +20:02:40.4: 14.37 +/- 0.06 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:53:42.07 +21:24:54.7: 14.52 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.06
Forced photometry reference-image weighted average: 15.13 +/- 0.10
Forced photometry reference-image weighted average: 14.62 +/- 0.06
Forced photometry reference-image weighted average: 14.63 +/- 0.06
Forced photometry reference-image weighted average: 14.75 +/- 0.07
Forced photometry reference-image weighted average: 15.55 +/- 0.14
Forced photometry reference-image weighted average: 15.21 +/- 0.10
Forced photometry filter REJECTED candidate at 03:22:43.63 +26:02:28.9: ref_mag=14.59 +/- 0.06 new_mean_mag=14.5275 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:59:28.44 +21:37:03.6: ref_mag=15.13 +/- 0.10 new_mean_mag=15.0705 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:30:09.23 +20:36:19.7: ref_mag=14.62 +/- 0.06 new_mean_mag=14.6135 delta=0.00 (need > 0.90)
Forced photometry reference-image weighted average: 14.54 +/- 0.05
Forced photometry filter REJECTED candidate at 03:23:57.21 +18:01:19.9: ref_mag=14.63 +/- 0.06 new_mean_mag=14.7230 delta=-0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:58:01.61 +19:39:53.5: ref_mag=14.75 +/- 0.07 new_mean_mag=15.0182 delta=-0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:27:30.81 +18:45:00.5: ref_mag=15.55 +/- 0.14 new_mean_mag=15.0365 delta=0.51 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:50:36.21 +23:12:30.6: ref_mag=15.21 +/- 0.10 new_mean_mag=15.1579 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 14.27 +/- 0.04
Forced photometry reference-image weighted average: 14.54 +/- 0.05
Forced photometry filter REJECTED candidate at 03:35:10.67 +20:29:07.3: ref_mag=14.54 +/- 0.05 new_mean_mag=14.6159 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:33:51.13 +20:02:40.4: ref_mag=14.27 +/- 0.04 new_mean_mag=14.4859 delta=-0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:53:42.07 +21:24:54.7: ref_mag=14.54 +/- 0.05 new_mean_mag=14.6534 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:45:12.28 +19:40:22.2: 13.59 +/- 0.03 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:29:06.95 +21:13:13.6: 13.41 +/- 0.02 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:54:14.81 +22:07:16.4: 14.18 +/- 0.06 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:29:29.49 +17:56:02.1: 14.20 +/- 0.06 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:23:56.72 +23:39:40.5: 13.95 +/- 0.05 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:30:51.58 +23:14:26.4: 13.61 +/- 0.03 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:44:08.56 +20:36:44.0: 13.99 +/- 0.04 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:37:19.87 +24:08:19.5: 14.15 +/- 0.05 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:45:46.17 +18:55:50.5: 12.67 +/- 0.01 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:45:12.28 +19:40:22.2: 13.66 +/- 0.03 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:54:14.81 +22:07:16.4: 14.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.02
Forced photometry filter REJECTED candidate at 03:45:12.28 +19:40:22.2: ref_mag=13.63 +/- 0.02 new_mean_mag=14.0854 delta=-0.46 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:23:56.72 +23:39:40.5: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.04
Forced photometry filter REJECTED candidate at 03:54:14.81 +22:07:16.4: ref_mag=14.18 +/- 0.04 new_mean_mag=14.4059 delta=-0.23 (need > 0.90)
Forced photometry reference-image weighted average: 13.97 +/- 0.03
Forced photometry filter REJECTED candidate at 03:23:56.72 +23:39:40.5: ref_mag=13.97 +/- 0.03 new_mean_mag=14.2563 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:37:19.87 +24:08:19.5: 14.12 +/- 0.05 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:30:51.58 +23:14:26.4: 13.62 +/- 0.03 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:29:06.95 +21:13:13.6: 13.50 +/- 0.03 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:29:29.49 +17:56:02.1: 14.15 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.03
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:44:08.56 +20:36:44.0: 13.93 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 03:37:19.87 +24:08:19.5: ref_mag=14.13 +/- 0.03 new_mean_mag=14.0997 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter REJECTED candidate at 03:30:51.58 +23:14:26.4: ref_mag=13.62 +/- 0.02 new_mean_mag=14.2215 delta=-0.60 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:29:06.95 +21:13:13.6: ref_mag=13.45 +/- 0.02 new_mean_mag=13.7896 delta=-0.34 (need > 0.90)
Forced photometry reference-image weighted average: 14.17 +/- 0.04
Forced photometry filter REJECTED candidate at 03:29:29.49 +17:56:02.1: ref_mag=14.17 +/- 0.04 new_mean_mag=14.4238 delta=-0.25 (need > 0.90)
Forced photometry reference-image weighted average: 13.96 +/- 0.03
Forced photometry filter REJECTED candidate at 03:44:08.56 +20:36:44.0: ref_mag=13.96 +/- 0.03 new_mean_mag=14.1316 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:26:56.89 +18:41:11.5: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:45:46.17 +18:55:50.5: 12.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Forced photometry filter REJECTED candidate at 03:45:46.17 +18:55:50.5: ref_mag=12.69 +/- 0.01 new_mean_mag=12.8987 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:26:56.89 +18:41:11.5: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:59:28.10 +17:48:09.5: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:30:52.21 +18:47:14.6: 14.07 +/- 0.06 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:34:23.83 +19:48:46.6: 14.25 +/- 0.07 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:25:07.11 +21:12:58.9: 14.31 +/- 0.07 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:25:11.65 +19:50:30.6: 14.14 +/- 0.05 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:26:34.37 +19:12:22.6: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:57:00.08 +21:54:20.8: 14.32 +/- 0.07 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:58:41.83 +23:51:23.2: 14.21 +/- 0.07 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:26:46.41 +22:44:39.1: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:59:28.10 +17:48:09.5: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:34:23.83 +19:48:46.6: 14.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.05
Forced photometry filter REJECTED candidate at 03:34:23.83 +19:48:46.6: ref_mag=14.26 +/- 0.05 new_mean_mag=14.2531 delta=0.00 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:30:52.21 +18:47:14.6: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.04
Forced photometry filter REJECTED candidate at 03:30:52.21 +18:47:14.6: ref_mag=14.07 +/- 0.04 new_mean_mag=14.0408 delta=0.03 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:25:11.65 +19:50:30.6: 14.21 +/- 0.05 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:25:07.11 +21:12:58.9: 14.37 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.04
Forced photometry filter REJECTED candidate at 03:25:11.65 +19:50:30.6: ref_mag=14.18 +/- 0.04 new_mean_mag=14.4575 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:26:34.37 +19:12:22.6: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:26:46.41 +22:44:39.1: 16.33 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.34 +/- 0.05
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:57:00.08 +21:54:20.8: 14.33 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 03:25:07.11 +21:12:58.9: ref_mag=14.34 +/- 0.05 new_mean_mag=14.3398 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:58:41.83 +23:51:23.2: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.05
Forced photometry filter REJECTED candidate at 03:57:00.08 +21:54:20.8: ref_mag=14.32 +/- 0.05 new_mean_mag=14.5018 delta=-0.18 (need > 0.90)
Forced photometry reference-image weighted average: 14.23 +/- 0.05
Forced photometry filter REJECTED candidate at 03:58:41.83 +23:51:23.2: ref_mag=14.23 +/- 0.05 new_mean_mag=14.3836 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:49:52.92 +21:09:08.7: 14.60 +/- 0.10 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:52:27.00 +18:35:16.8: 14.27 +/- 0.07 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:50:45.98 +26:01:57.7: 14.59 +/- 0.09 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:44:01.68 +18:45:37.1: 14.60 +/- 0.09 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:37:51.71 +26:01:42.0: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:52:18.85 +24:24:42.7: 14.58 +/- 0.09 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:49:52.92 +21:09:08.7: 14.47 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.06
Forced photometry filter REJECTED candidate at 03:49:52.92 +21:09:08.7: ref_mag=14.53 +/- 0.06 new_mean_mag=14.5240 delta=0.00 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:52:27.00 +18:35:16.8: 14.43 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.05
Forced photometry filter REJECTED candidate at 03:52:27.00 +18:35:16.8: ref_mag=14.34 +/- 0.05 new_mean_mag=14.4700 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:37:51.71 +26:01:42.0: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:50:45.98 +26:01:57.7: 14.58 +/- 0.09 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:44:01.68 +18:45:37.1: 15.00 +/- 0.12 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:52:18.85 +24:24:42.7: 14.67 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.06
Forced photometry filter REJECTED candidate at 03:50:45.98 +26:01:57.7: ref_mag=14.58 +/- 0.06 new_mean_mag=14.6302 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 14.73 +/- 0.07
Forced photometry reference-image weighted average: 14.62 +/- 0.06
Forced photometry filter REJECTED candidate at 03:44:01.68 +18:45:37.1: ref_mag=14.73 +/- 0.07 new_mean_mag=14.7907 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:52:18.85 +24:24:42.7: ref_mag=14.62 +/- 0.06 new_mean_mag=14.6678 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:49:32.84 +19:11:29.9: 14.94 +/- 0.12 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:44:57.55 +22:17:06.3: 14.96 +/- 0.14 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:45:30.91 +20:57:22.9: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:59:32.39 +22:13:07.9: 15.10 +/- 0.13 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:59:11.15 +19:16:40.7: 14.79 +/- 0.12 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:49:32.84 +19:11:29.9: 15.13 +/- 0.13 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.09
Forced photometry filter REJECTED candidate at 03:49:32.84 +19:11:29.9: ref_mag=15.02 +/- 0.09 new_mean_mag=14.8949 delta=0.13 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:44:57.55 +22:17:06.3: 14.94 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.10
Forced photometry filter REJECTED candidate at 03:44:57.55 +22:17:06.3: ref_mag=14.95 +/- 0.10 new_mean_mag=14.7986 delta=0.15 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:59:11.15 +19:16:40.7: 14.90 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.09
Forced photometry filter REJECTED candidate at 03:59:11.15 +19:16:40.7: ref_mag=14.84 +/- 0.09 new_mean_mag=14.8656 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:45:30.91 +20:57:22.9: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:59:32.39 +22:13:07.9: 14.94 +/- 0.11 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.09
Forced photometry filter REJECTED candidate at 03:59:32.39 +22:13:07.9: ref_mag=15.01 +/- 0.09 new_mean_mag=14.8839 delta=0.13 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:44:24.76 +24:46:03.9: 14.99 +/- 0.13 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:47:01.16 +23:58:18.0: 14.99 +/- 0.14 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:44:12.77 +20:24:15.1: 15.20 +/- 0.14 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:39:58.18 +18:23:34.3: 15.21 +/- 0.14 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:44:24.76 +24:46:03.9: 14.91 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.09
Forced photometry filter REJECTED candidate at 03:44:24.76 +24:46:03.9: ref_mag=14.95 +/- 0.09 new_mean_mag=15.0161 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:47:01.16 +23:58:18.0: 15.06 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.10
Forced photometry filter REJECTED candidate at 03:47:01.16 +23:58:18.0: ref_mag=15.03 +/- 0.10 new_mean_mag=14.7775 delta=0.25 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:44:12.77 +20:24:15.1: 15.08 +/- 0.12 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.09
Forced photometry filter REJECTED candidate at 03:44:12.77 +20:24:15.1: ref_mag=15.13 +/- 0.09 new_mean_mag=15.0471 delta=0.09 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:39:58.18 +18:23:34.3: 15.04 +/- 0.13 detection
Forced photometry reference-image weighted average: 15.11 +/- 0.09
Forced photometry filter REJECTED candidate at 03:39:58.18 +18:23:34.3: ref_mag=15.11 +/- 0.09 new_mean_mag=15.0603 delta=0.05 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:27:13.93 +24:31:19.1: 15.60 +/- 0.20 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:49:47.35 +23:40:36.0: 15.03 +/- 0.14 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:48:13.56 +19:51:04.8: 15.40 +/- 0.18 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:27:13.93 +24:31:19.1: 15.49 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.54 +/- 0.13
Forced photometry filter REJECTED candidate at 03:27:13.93 +24:31:19.1: ref_mag=15.54 +/- 0.13 new_mean_mag=15.1129 delta=0.43 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:59:26.82 +25:50:20.8: 14.93 +/- 0.14 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:49:47.35 +23:40:36.0: 15.07 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.11
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:48:13.56 +19:51:04.8: 15.47 +/- 0.20 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:59:26.82 +25:50:20.8: 15.04 +/- 0.15 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:50:27.64 +19:05:29.8: 15.44 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 03:49:47.35 +23:40:36.0: ref_mag=15.05 +/- 0.11 new_mean_mag=14.9775 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 14.98 +/- 0.10
Forced photometry reference-image weighted average: 15.43 +/- 0.13
Forced photometry filter REJECTED candidate at 03:59:26.82 +25:50:20.8: ref_mag=14.98 +/- 0.10 new_mean_mag=15.1614 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:48:13.56 +19:51:04.8: ref_mag=15.43 +/- 0.13 new_mean_mag=15.1701 delta=0.26 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:50:27.64 +19:05:29.8: 15.51 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.47 +/- 0.13
Forced photometry filter REJECTED candidate at 03:50:27.64 +19:05:29.8: ref_mag=15.47 +/- 0.13 new_mean_mag=15.2170 delta=0.25 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:52:23.27 +25:51:24.5: 15.58 +/- 0.22 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:42:43.21 +24:17:31.2: 15.27 +/- 0.16 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:52:23.27 +25:51:24.5: 15.36 +/- 0.17 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:56:35.68 +25:23:16.6: 14.95 +/- 0.13 detection
Forced photometry reference-image weighted average: 15.44 +/- 0.13
Forced photometry filter REJECTED candidate at 03:52:23.27 +25:51:24.5: ref_mag=15.44 +/- 0.13 new_mean_mag=15.0132 delta=0.43 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:42:43.21 +24:17:31.2: 15.19 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.10
Forced photometry filter REJECTED candidate at 03:42:43.21 +24:17:31.2: ref_mag=15.23 +/- 0.10 new_mean_mag=15.1446 delta=0.08 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:56:35.68 +25:23:16.6: 14.87 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.08
Forced photometry filter REJECTED candidate at 03:56:35.68 +25:23:16.6: ref_mag=14.90 +/- 0.08 new_mean_mag=15.2082 delta=-0.31 (need > 0.90)
Adding exclusion_list_local.txt__out88368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95210.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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: 5s
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Considering the candidate 86071_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86071_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86075_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86075_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86081_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86081_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86083_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86083_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86090_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86090_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86093_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86093_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86096_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86096_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86100_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86100_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86103_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86103_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86105_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86105_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86109_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86109_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86111_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86111_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86113_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86113_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86117_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86117_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86119_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86119_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86120_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86120_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86121_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86121_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
**** FOUND 03:30:46.26 +17:48:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86122_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86122_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86128_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86128_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 86129_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86129_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
**** FOUND 03:52:57.53 +19:16:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86130_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 86130_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 87763_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 87763_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
**** FOUND 03:37:11.52 +21:03:14.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 88368_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
Preparing report for the candidate 88368_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
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Considering the candidate 89173_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 89173_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
**** FOUND 03:55:12.99 +23:36:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89211_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 89211_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
**** FOUND 03:36:51.44 +23:11:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89430_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
Preparing report for the candidate 89430_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
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Considering the candidate 90374_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 90374_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
**** FOUND 03:56:36.97 +25:08:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91012_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 91012_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
**** FOUND 03:24:20.77 +24:45:10.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 91026_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 91026_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
**** FOUND 03:51:15.11 +24:34:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91584_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 91584_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 91987_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 91987_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 92626_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 92626_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 92800_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 92800_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 93224_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
Preparing report for the candidate 93224_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
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Considering the candidate 93247_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
Preparing report for the candidate 93247_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
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Considering the candidate 93309_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 93309_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 93347_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 93347_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 93511_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 93511_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 93674_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 93674_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 93757_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 93757_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 94355_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 94355_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 94437_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 94437_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 94535_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
Preparing report for the candidate 94535_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
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Considering the candidate 94623_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 94623_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 94841_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 94841_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 95210_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
Preparing report for the candidate 95210_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
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Considering the candidate 95254_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 95254_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 95318_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 95318_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 95473_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 95473_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 95667_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 95667_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 95699_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 95699_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 95707_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 95707_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 96041_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 96041_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 96112_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 96112_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 96218_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 96218_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 96272_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 96272_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 96273_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 96273_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 96290_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 96290_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
**** FOUND 03:42:10.71 +19:42:29.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 96297_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 96297_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 96302_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 96302_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 96348_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 96348_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
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Considering the candidate 96404_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368
The candidate 96404_fd_Tau-02-Q2b1x1_2026-09-09_05-44-44_20.00sec_-0.00C_LIGHT_0368 did not pass the final checks
