This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 15.3840* 04 12 29.08 +20 58 53.4 7.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461267.8840,7.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260815.3840 7.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 15.3840 2461267.8840 11.95 04:17:33.89 +24:26:38.2
171.61714 -18.38088 galactic Tau Second-epoch detections are separated by 0.6" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.230 Athamantis 1 0 1 12.2 0 0
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:17:33.89 +24:26:38.2: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:17:33.89 +24:26:38.2: 15.96 +/- 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 08 15.3840* 04 17 33.89 +24 26 38.2 11.9 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,2461267.8840,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260815.3840 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 15.3840* 04 12 29.08 +20 58 53.3 7.4 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,2461267.8840,7.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260815.3840 7.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 15.3840 2461267.8840 12.85 04:08:58.02 +23:55:06.9
170.59548 -20.16718 galactic Tau Second-epoch detections are separated by 0.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.49 Pales -0 -0 0 13.0 0 0
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:08:58.02 +23:55:06.9: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:08:58.02 +23:55:06.9: 15.91 +/- 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 08 15.3840* 04 08 58.02 +23 55 06.9 12.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461267.8840,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260815.3840 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 15.3840 2461267.8840 13.69 04:21:57.19 +23:51:31.2
172.78236 -18.03525 galactic Tau Second-epoch detections are separated by 1.8" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.714 Ulula -0 -1 1 14.1 -0 0
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:57.19 +23:51:31.2: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:21:57.19 +23:51:31.2: 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 08 15.3840* 04 21 57.19 +23 51 31.2 13.7 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,2461267.8840,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260815.3840 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 15.3840 2461267.8840 13.35 05:06:00.56 +22:56:06.2
180.06116 -10.73092 galactic Tau Second-epoch detections are separated by 1.5" and 2.3 pix
The object was found in VSX20" Gaia DR3 3418391481939007488
Type: RS
# Max. Min./Amp. JD0 Period
15.960 G 16.060 G K
The object was found in astcheck.110 Lydia 0 -0 1 13.3 0 0
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:00.56 +22:56:06.2: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:00.56 +22:56:06.2: 16.05 +/- 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 08 15.3840* 05 06 00.56 +22 56 06.2 13.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3418391481939007488,2461267.8840,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3418391481939007488 20260815.3840 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 15.3840 2461267.8840 13.67 04:18:01.28 +20:33:05.2
174.75384 -20.91830 galactic Tau Second-epoch detections are separated by 1.2" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.344 Desiderata -0 -0 0 13.8 0 0
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:18:01.28 +20:33:05.2: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:18:01.28 +20:33:05.2: 16.17 +/- 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 08 15.3840* 04 18 01.28 +20 33 05.2 13.7 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,2461267.8840,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260815.3840 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 15.3840 2461267.8840 14.40 04:23:35.17 +25:48:00.6
171.53242 -16.45988 galactic Tau Second-epoch detections are separated by 2.1" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.359 Georgia -1 -0 1 14.5 0 0
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:23:35.17 +25:48:00.6: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:23:35.17 +25:48:00.6: 16.14 +/- 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 08 15.3840* 04 23 35.17 +25 48 00.6 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,2461267.8840,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260815.3840 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 15.3840 2461267.8840 14.32 04:14:07.41 +21:05:18.8
173.67279 -21.23542 galactic Tau Second-epoch detections are separated by 1.8" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.631 Philippina -1 0 1 14.2 0 0
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:14:07.41 +21:05:18.8: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:14:07.41 +21:05:18.8: 16.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 15.3840* 04 14 07.41 +21 05 18.8 14.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461267.8840,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260815.3840 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 15.3840 2461267.8840 14.45 04:29:23.55 +24:15:44.4
173.64229 -16.49492 galactic Tau Second-epoch detections are separated by 0.9" and 1.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.422 Berolina -1 -0 1 14.8 0 0
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:29:23.55 +24:15:44.4: 16.34 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:29:23.55 +24:15:44.4: 16.20 +/- 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 08 15.3840* 04 29 23.55 +24 15 44.4 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,2461267.8840,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260815.3840 14.45CV 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: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461267.88426810 15.08.2026 09:13:10.764 /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 8 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): 10808
Objects passed selection criteria: 10781
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 9303.25
Average stars matched: 9169 (98.557 %)
Memory usage VmPeak: 236884 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 15 04:34:30 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: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461267.88426810 15.08.2026 09:13:10.764 /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 140
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.21
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: 29 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): 76334
Objects passed selection criteria: 76201
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 62143.5
Average stars matched: 60647 (97.5919 %)
Memory usage VmPeak: 563876 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 15 04:37:03 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
SExtractor catalog cache: saved Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.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: 2461267.88377429
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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits exists and is non-empty
wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (1st reference image)
verification OK: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:56.045 +21:59:37.33 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-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits (1st new image)
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
Image size: 941.8'x626.7' 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: 04:36:59.214 +21:59:52.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:36:56.045 +21:59:37.33
Second-epoch image center 04:36:59.214 +21:59:52.26
Angular distance between the image centers 0.0129 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits (2nd new image)
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
Image size: 941.8'x626.7' 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: 04:36:58.345 +21:59:52.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:36:56.045 +21:59:37.33
Second-epoch image center 04:36:58.345 +21:59:52.39
Angular distance between the image centers 0.0098 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 04:36:59.214 +21:59:52.26
Second-epoch second image center 04:36:58.345 +21:59:52.39
Angular distance between the image centers 0.00336 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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.HobD0AMvXV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.I0jEaWcmiY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits &> /tmp/tmp.qPlSwXYG01
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits &> /tmp/tmp.xWNDlzavqT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Found non-empty wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
The reference image (wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat) found
'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat' -> 'wcsmag.cat'
Read 11927 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5112 to 78.0902 deg, Dec +16.4856 to +27.2829 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 60.5112 to 78.0902 deg, Dec 16.4856 to 27.2829 deg
Loaded 5180 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): 3947 out of 4318 total matches.
Matched with Tycho-2 4318 out of 11927 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.997400
a=0.000000 b=1.000000 c=22.997400
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11927 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5112 to 78.0902 deg, Dec +16.4856 to +27.2829 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 60.5112 to 78.0902 deg, Dec 16.4856 to 27.2829 deg
Loaded 5180 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): 3947 out of 4318 total matches.
Matched with Tycho-2 4318 out of 11927 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Forced-photometry filter: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -> calib.txt_param_ref_wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (aperture=6.0)
Read 11076 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5314 to 78.0905 deg, Dec +16.4856 to +27.2796 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 60.5314 to 78.0905 deg, Dec 16.4856 to 27.2796 deg
Loaded 5169 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): 3956 out of 4300 total matches.
Matched with Tycho-2 4300 out of 11076 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Forced-photometry filter: calibrated wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits -> calib.txt_param_ref_wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
2.1 pix Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
3.1 pix fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
3.1 pix fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
Limiting magnitude estimates:
15.5 mag. Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.4 mag. Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
14.5 mag. fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
14.5 mag. fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.HobD0AMvXV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=967, bad_region=0, passed=11927
Got 11927 stars (including 10942 good ones) from the SExtractor catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
util/solve_plate_with_UCAC5 got 11927 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4866 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 4844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11927 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 4866 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4844 stars left (next iteration limit 5328)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits N_match=4844 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.308 sigma_q3_arcsec=0.262 sigma_q4_arcsec=0.246 n_q1=1283 n_q2=1077 n_q3=1448 n_q4=1036 worst_quadrant_to_overall_ratio=1.251
The image catalog is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.I0jEaWcmiY (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.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-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits' -> 'wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.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-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=897, bad_region=0, passed=11076
Got 11076 stars (including 10166 good ones) from the SExtractor catalog wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat
util/solve_plate_with_UCAC5 got 11076 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 4844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11076 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11076 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11076 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4844 stars left (next iteration limit 5328)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits N_match=4844 sigma_overall_arcsec=0.351 sigma_q1_arcsec=0.456 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.285 n_q1=1273 n_q2=1107 n_q3=1409 n_q4=1055 worst_quadrant_to_overall_ratio=1.297
The image catalog is written to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qPlSwXYG01 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
Checking if the catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
WCS catalog name: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=370, bad_region=0, passed=7202
Got 7202 stars (including 6823 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat
util/solve_plate_with_UCAC5 got 7202 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4858 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 4835 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 7202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4855 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 7202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 7202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4834 stars left (next iteration limit 5318)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4834 robust_rms=12.707 arcsec worst_quadrant_rms=13.643 arcsec
SIP_REFIT: SIP order 3 trial: matched=4834 robust_rms=0.425 arcsec worst_quadrant_rms=0.467 arcsec
SIP_REFIT: SIP order 5 trial: matched=4834 robust_rms=0.343 arcsec worst_quadrant_rms=0.392 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4834 robust_rms_before=1.030 arcsec robust_rms_before_corrected=0.352 arcsec robust_rms_after=0.343 arcsec worst_quadrant_rms_before=0.419 worst_quadrant_rms_after=0.392
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.419 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits N_match=4834 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.338 sigma_q2_arcsec=0.406 sigma_q3_arcsec=0.298 sigma_q4_arcsec=0.341 n_q1=1109 n_q2=1274 n_q3=1143 n_q4=1308 worst_quadrant_to_overall_ratio=1.154
The image catalog is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits -region wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.xWNDlzavqT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
Checking if the catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
WCS catalog name: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=365, bad_region=0, passed=7236
Got 7236 stars (including 6865 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat
util/solve_plate_with_UCAC5 got 7236 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4855 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 4831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 7236 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4852 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 7236 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 7236 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4829 stars left (next iteration limit 5314)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4829 robust_rms=12.816 arcsec worst_quadrant_rms=13.973 arcsec
SIP_REFIT: SIP order 3 trial: matched=4829 robust_rms=0.429 arcsec worst_quadrant_rms=0.465 arcsec
SIP_REFIT: SIP order 5 trial: matched=4829 robust_rms=0.340 arcsec worst_quadrant_rms=0.394 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4829 robust_rms_before=1.024 arcsec robust_rms_before_corrected=0.349 arcsec robust_rms_after=0.340 arcsec worst_quadrant_rms_before=0.417 worst_quadrant_rms_after=0.394
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.417 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits N_match=4829 sigma_overall_arcsec=0.342 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.299 sigma_q4_arcsec=0.352 n_q1=1105 n_q2=1273 n_q3=1149 n_q4=1302 worst_quadrant_to_overall_ratio=1.173
The image catalog is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits -region wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits to local_wcs_cache/
'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'local_wcs_cache/wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
Saving the final (post-refit) wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits to local_wcs_cache/
'wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits' -> 'local_wcs_cache/wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits'
Saving the final (post-refit) wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits'
Saving the final (post-refit) wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits sigma_overall=0.304 worst_q_ratio=1.251
ref2=Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits sigma_overall=0.351 worst_q_ratio=1.297
new1=fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits sigma_overall=0.352 worst_q_ratio=1.154
new2=fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits sigma_overall=0.342 worst_q_ratio=1.173
reference average sigma_overall=0.3275 worst_q_ratio=1.274
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161_astrometric_residuals.png (4844 matched stars from wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202_astrometric_residuals.png (4844 matched stars from wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354_astrometric_residuals.png (4834 matched stars from wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355_astrometric_residuals.png (4829 matched stars from wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits'
Saving fully-calibrated image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits'
Preparing the HTML report for the field Tau-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:33:52.04 +22:50:29.8: 12.89 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:17:33.89 +24:26:38.2: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:17:33.89 +24:26:38.2: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:33:52.04 +22:50:29.8: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter REJECTED candidate at 04:33:52.04 +22:50:29.8: ref_mag=12.73 +/- 0.01 new_mean_mag=12.1763 delta=0.56 (need > 0.90)
Adding exclusion_list_local.txt__out20472.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 68s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20365_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 20365_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:23:57.82 +24:18:13.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20367_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 20367_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20472_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 20472_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20514_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 20514_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04887_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 04887_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:44:21.54 +22:50:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07981_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 07981_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:21:25.46 +20:15:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10554_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 10554_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:52:02.24 +17:32:18.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 70s
Prepared the HTML report for the field Tau-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:17:33.89 +24:26:38.2
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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
SExtractor catalog cache: saved Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Creating symlink local_wcs_cache/wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits exists and is non-empty
wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (1st reference image)
verification OK: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:56.045 +21:59:37.33 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-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits (1st new image)
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
Image size: 941.8'x626.7' 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: 04:36:59.214 +21:59:52.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:36:56.045 +21:59:37.33
Second-epoch image center 04:36:59.214 +21:59:52.26
Angular distance between the image centers 0.0129 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits (2nd new image)
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
Image size: 941.8'x626.7' 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: 04:36:58.345 +21:59:52.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:36:56.045 +21:59:37.33
Second-epoch image center 04:36:58.345 +21:59:52.39
Angular distance between the image centers 0.0098 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 04:36:59.214 +21:59:52.26
Second-epoch second image center 04:36:58.345 +21:59:52.39
Angular distance between the image centers 0.00336 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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.6puhiv6rmw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.Xxf0TR47OL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits &> /tmp/tmp.z5jbSQC8YH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits &> /tmp/tmp.0E2E2PQZ5E
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Found non-empty wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
The reference image (wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat) found
'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat' -> 'wcsmag.cat'
Read 86341 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5065 to 78.1101 deg, Dec +16.4673 to +27.2853 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 60.5065 to 78.1101 deg, Dec 16.4673 to 27.2853 deg
Loaded 5193 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): 3472 out of 4349 total matches.
Matched with Tycho-2 4349 out of 86341 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.857350
a=0.000000 b=1.000000 c=22.857350
From vast_summary.log: estimated ref. image limiting mag.: -7.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.65
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.65
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 86341 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5065 to 78.1101 deg, Dec +16.4673 to +27.2853 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 60.5065 to 78.1101 deg, Dec 16.4673 to 27.2853 deg
Loaded 5193 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): 3472 out of 4349 total matches.
Matched with Tycho-2 4349 out of 86341 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Forced-photometry filter: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -> calib.txt_param_ref_wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (aperture=4.5)
Read 80651 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5064 to 78.1103 deg, Dec +16.4671 to +27.2945 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 60.5064 to 78.1103 deg, Dec 16.4671 to 27.2945 deg
Loaded 5197 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): 3489 out of 4349 total matches.
Matched with Tycho-2 4349 out of 80651 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Forced-photometry filter: calibrated wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits -> calib.txt_param_ref_wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 131 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
1.9 pix Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
2.9 pix fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
2.9 pix fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
Limiting magnitude estimates:
15.7 mag. Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.5 mag. Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
14.6 mag. fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
14.6 mag. fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.1 (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.6puhiv6rmw (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=6242, bad_region=8, passed=86318
Got 86318 stars (including 79890 good ones) from the SExtractor catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
util/solve_plate_with_UCAC5 got 86318 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 4857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 86318 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 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 86318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 86318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4857 stars left (next iteration limit 5342)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits N_match=4857 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.254 n_q1=1260 n_q2=1091 n_q3=1439 n_q4=1067 worst_quadrant_to_overall_ratio=1.279
The image catalog is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Xxf0TR47OL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.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-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits' -> 'wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.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-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=5759, bad_region=1, passed=80631
Got 80631 stars (including 74709 good ones) from the SExtractor catalog wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat
util/solve_plate_with_UCAC5 got 80631 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 4855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 80631 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 80631 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 80631 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4855 stars left (next iteration limit 5340)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.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-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits N_match=4855 sigma_overall_arcsec=0.336 sigma_q1_arcsec=0.428 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.316 sigma_q4_arcsec=0.269 n_q1=1222 n_q2=1136 n_q3=1399 n_q4=1098 worst_quadrant_to_overall_ratio=1.273
The image catalog is written to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.z5jbSQC8YH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
Checking if the catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
WCS catalog name: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1727, bad_region=20, passed=41572
Got 41572 stars (including 39767 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat
util/solve_plate_with_UCAC5 got 41572 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 4863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 4847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 41571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4846 matched stars entering correct_measured_positions(), 41571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4846 matched stars entering correct_measured_positions(), 41571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4846 stars left (next iteration limit 5331)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.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=4846 robust_rms=12.561 arcsec worst_quadrant_rms=13.206 arcsec
SIP_REFIT: SIP order 3 trial: matched=4846 robust_rms=0.422 arcsec worst_quadrant_rms=0.460 arcsec
SIP_REFIT: SIP order 5 trial: matched=4846 robust_rms=0.341 arcsec worst_quadrant_rms=0.391 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4846 robust_rms_before=1.026 arcsec robust_rms_before_corrected=0.349 arcsec robust_rms_after=0.341 arcsec worst_quadrant_rms_before=0.439 worst_quadrant_rms_after=0.391
SIP_REFIT: applied the refit solution to the output catalog positions only (order 5, robust RMS 1.026 -> 0.341 arcsec); the image header was NOT rewritten as wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits is a symbolic link
WCS_QUALITY_DIAG: file=fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits N_match=4846 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.421 sigma_q3_arcsec=0.315 sigma_q4_arcsec=0.370 n_q1=1116 n_q2=1234 n_q3=1190 n_q4=1306 worst_quadrant_to_overall_ratio=1.170
The image catalog is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits -region wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0E2E2PQZ5E (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
Checking if the catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
WCS catalog name: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1774, bad_region=26, passed=41736
Got 41736 stars (including 39891 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat
util/solve_plate_with_UCAC5 got 41736 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4842 matched stars entering correct_measured_positions(), 4842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4842 matched stars entering correct_measured_positions(), 41734 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4842 matched stars entering correct_measured_positions(), 41734 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4842 matched stars entering correct_measured_positions(), 41734 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4842 stars left (next iteration limit 5326)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.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=4842 robust_rms=12.691 arcsec worst_quadrant_rms=13.428 arcsec
SIP_REFIT: SIP order 3 trial: matched=4842 robust_rms=0.436 arcsec worst_quadrant_rms=0.480 arcsec
SIP_REFIT: SIP order 5 trial: matched=4842 robust_rms=0.338 arcsec worst_quadrant_rms=0.396 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4842 robust_rms_before=1.019 arcsec robust_rms_before_corrected=0.348 arcsec robust_rms_after=0.338 arcsec worst_quadrant_rms_before=0.426 worst_quadrant_rms_after=0.396
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.426 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits N_match=4842 sigma_overall_arcsec=0.343 sigma_q1_arcsec=0.312 sigma_q2_arcsec=0.426 sigma_q3_arcsec=0.292 sigma_q4_arcsec=0.350 n_q1=1129 n_q2=1222 n_q3=1183 n_q4=1308 worst_quadrant_to_overall_ratio=1.242
The image catalog is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits -region wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-12-28_20.00sec_-0.00C_LIGHTs_0354.fits
Saving fully-calibrated image wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-15_CI_Tau-03-Q1b1x1_041548_TTUQ1b1x1_2858789_Tl9UDW0x/wcs_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355.fits
Preparing the HTML report for the field Tau-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:08:04.11 +22:13:52.6: 13.08 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:24:41.31 +25:30:53.7: 13.88 +/- 0.04 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:15:25.30 +20:13:12.2: 13.90 +/- 0.04 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:09:08.02 +21:52:56.8: 12.48 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:19:34.13 +18:12:35.0: 14.13 +/- 0.05 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:14:36.77 +20:32:29.4: 13.18 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:09:51.89 +26:34:06.4: 13.41 +/- 0.03 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:08:04.11 +22:13:52.6: 13.00 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:14:36.77 +20:32:29.4: 13.10 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:24:41.31 +25:30:53.7: 13.85 +/- 0.04 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:15:25.30 +20:13:12.2: 13.84 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:09:51.89 +26:34:06.4: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter REJECTED candidate at 04:08:04.11 +22:13:52.6: ref_mag=13.05 +/- 0.02 new_mean_mag=13.2145 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:19:34.13 +18:12:35.0: 14.05 +/- 0.06 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:09:08.02 +21:52:56.8: 12.49 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 04:14:36.77 +20:32:29.4: ref_mag=13.14 +/- 0.02 new_mean_mag=13.1255 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Forced photometry filter REJECTED candidate at 04:24:41.31 +25:30:53.7: ref_mag=13.87 +/- 0.03 new_mean_mag=14.0192 delta=-0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:15:25.30 +20:13:12.2: ref_mag=13.87 +/- 0.03 new_mean_mag=13.8113 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry reference-image weighted average: 14.09 +/- 0.04
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter REJECTED candidate at 04:09:51.89 +26:34:06.4: ref_mag=13.38 +/- 0.02 new_mean_mag=13.6766 delta=-0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:19:34.13 +18:12:35.0: ref_mag=14.09 +/- 0.04 new_mean_mag=14.2009 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:09:08.02 +21:52:56.8: ref_mag=12.48 +/- 0.01 new_mean_mag=12.5926 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:08:58.02 +23:55:06.9: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:45.27 +19:28:44.2: 12.50 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:08:58.02 +23:55:06.9: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:21:45.27 +19:28:44.2: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 04:21:45.27 +19:28:44.2: ref_mag=12.49 +/- 0.01 new_mean_mag=12.3940 delta=0.09 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:55:44.25 +20:00:57.7: 13.06 +/- 0.03 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:55:44.25 +20:00:57.7: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter REJECTED candidate at 04:55:44.25 +20:00:57.7: ref_mag=13.09 +/- 0.02 new_mean_mag=13.0904 delta=0.00 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:38:35.46 +17:25:28.6: 13.47 +/- 0.03 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:57.19 +23:51:31.2: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:09:56.31 +21:49:36.2: 13.44 +/- 0.04 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:00.56 +22:56:06.2: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:18:01.28 +20:33:05.2: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:38:35.46 +17:25:28.6: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter REJECTED candidate at 04:38:35.46 +17:25:28.6: ref_mag=13.50 +/- 0.02 new_mean_mag=13.3149 delta=0.18 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:21:57.19 +23:51:31.2: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:08:41.37 +22:15:33.7: 14.05 +/- 0.06 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:09:56.31 +21:49:36.2: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter REJECTED candidate at 05:09:56.31 +21:49:36.2: ref_mag=13.45 +/- 0.03 new_mean_mag=13.3419 delta=0.11 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:06:00.56 +22:56:06.2: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:18:01.28 +20:33:05.2: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:08:41.37 +22:15:33.7: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.04
Forced photometry filter REJECTED candidate at 04:08:41.37 +22:15:33.7: ref_mag=14.01 +/- 0.04 new_mean_mag=13.8430 delta=0.16 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:03:15.34 +20:54:49.9: 13.84 +/- 0.06 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:20:37.36 +19:15:34.6: 14.08 +/- 0.05 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 05:03:15.34 +20:54:49.9: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Forced photometry filter REJECTED candidate at 05:03:15.34 +20:54:49.9: ref_mag=13.85 +/- 0.04 new_mean_mag=13.6561 delta=0.20 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:20:37.36 +19:15:34.6: 14.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Forced photometry filter REJECTED candidate at 04:20:37.36 +19:15:34.6: ref_mag=14.10 +/- 0.04 new_mean_mag=13.9670 delta=0.13 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:19:13.92 +23:20:36.9: 14.36 +/- 0.08 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:23:35.17 +25:48:00.6: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:33:31.23 +24:17:47.2: 14.23 +/- 0.06 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:19:13.92 +23:20:36.9: 14.46 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.06
Forced photometry filter REJECTED candidate at 04:19:13.92 +23:20:36.9: ref_mag=14.40 +/- 0.06 new_mean_mag=14.3733 delta=0.03 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:23:35.17 +25:48:00.6: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:33:31.23 +24:17:47.2: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Forced photometry filter REJECTED candidate at 04:33:31.23 +24:17:47.2: ref_mag=14.20 +/- 0.04 new_mean_mag=14.1794 delta=0.02 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:14:07.41 +21:05:18.8: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:29:23.55 +24:15:44.4: 16.34 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:14:07.41 +21:05:18.8: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:29:23.55 +24:15:44.4: 16.20 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out101443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102148.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 65s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101179_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101179_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101182_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101182_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101184_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101184_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:19:18.00 +25:53:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101189_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101189_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:31:44.25 +25:22:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101192_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101192_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101193_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101193_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101200_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101200_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101202_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101202_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101203_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101203_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101204_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101204_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101205_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101205_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:06:31.47 +22:04:42.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101206_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101206_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:23:57.80 +24:18:13.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101208_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 101208_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101260_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101260_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101274_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101274_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:28:23.70 +19:10:45.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101286_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101286_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101291_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101291_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101295_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101295_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101311_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101311_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101317_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101317_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:17:33.89 +24:26:38.2 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101358_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101358_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101386_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101386_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101395_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101395_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101412_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101412_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101427_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101427_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101441_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101441_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101443_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 101443_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101445_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101445_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:42:09.70 +22:55:08.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101447_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101447_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101449_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101449_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101462_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101462_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:26:29.16 +22:48:44.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101470_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101470_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:10:47.87 +18:26:18.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101472_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101472_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:05:06.82 +23:48:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101502_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101502_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:34:38.43 +22:42:10.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101558_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101558_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:57:57.04 +23:57:20.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101574_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101574_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101579_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101579_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:57:47.86 +23:58:34.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101587_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101587_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101592_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101592_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:03:20.98 +23:48:38.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101626_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101626_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:21:32.79 +21:00:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101629_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101629_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:36:30.03 +23:18:39.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101633_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101633_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:42:24.66 +22:56:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101639_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101639_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:11:19.42 +24:25:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101648_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101648_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:20:33.74 +25:48:34.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101650_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101650_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:55:45.29 +19:58:58.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101655_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101655_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:19:40.57 +23:44:17.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101665_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101665_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101666_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101666_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101676_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101676_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:25:20.75 +22:10:33.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101680_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101680_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:28:27.12 +19:11:36.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101687_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101687_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101708_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101708_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101716_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101716_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101725_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101725_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101739_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101739_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101750_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101750_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101755_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101755_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:32:38.92 +23:58:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101764_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101764_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101769_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101769_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:36:07.91 +21:31:43.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101773_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101773_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:04:52.76 +23:55:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101774_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101774_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:19:30.10 +21:45:12.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101778_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101778_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101781_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101781_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101786_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101786_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101790_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101790_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101798_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101798_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101802_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 101802_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101806_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101806_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101807_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101807_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101821_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 101821_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101828_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 101828_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101837_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101837_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:28:14.46 +24:06:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101849_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101849_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:55:16.56 +21:52:00.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101876_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101876_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101891_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101891_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101905_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101905_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101910_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101910_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101913_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101913_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:23:18.68 +21:23:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101917_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101917_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:23:58.74 +24:19:30.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101922_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101922_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101936_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101936_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101943_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101943_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101945_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101945_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101947_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101947_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101949_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101949_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101959_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101959_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101965_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101965_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101980_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101980_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101993_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 101993_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102021_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102021_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102031_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102031_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102036_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102036_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102038_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102038_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102039_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102039_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102045_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102045_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102048_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102048_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102050_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102050_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:29:54.29 +26:03:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102055_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102055_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102058_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102058_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102067_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102067_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102072_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 102072_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102073_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102073_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102074_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102074_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102080_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102080_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102087_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102087_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102090_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102090_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102094_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102094_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102096_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102096_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102100_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102100_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102103_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102103_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102109_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102109_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102114_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102114_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102122_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 102122_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102131_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102131_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102138_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102138_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102139_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102139_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102148_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 102148_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102156_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102156_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:38:35.02 +20:26:21.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102166_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 102166_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37500_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 37500_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:32:48.10 +22:39:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58469_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 58469_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:52:46.96 +17:16:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53022_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 53022_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:58:39.82 +20:57:06.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70750_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 70750_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:17:46.12 +18:22:37.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80328_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 80328_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:02:18.25 +18:20:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36988_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 36988_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:46:31.87 +22:41:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35380_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 35380_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:44:21.52 +22:50:08.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05458_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 05458_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:09:07.04 +26:08:16.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60271_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 60271_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:21:25.47 +20:15:59.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65103_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 65103_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:52:02.24 +17:32:18.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15632_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 15632_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:44:35.08 +25:01:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08495_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355
The candidate 08495_fd_Tau-03-Q1b1x1_2026-08-15_04-13-10_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
