This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY
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 07.3983* 05 46 53.54 +23 34 47.6 6.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461259.8983,6.63,0.05,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 20260807.3983 6.63CV 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 07.3983* 05 21 07.66 +23 38 19.9 10.7 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
target,2461259.8983,10.68,0.05,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
target 20260807.3983 10.68CV 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 07.3983 2461259.8983 9.28 05:50:00.92 +22:08:15.8
186.33512 -2.66368 galactic Ori Second-epoch detections are separated by 1.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1 Ceres 0 0 0 9.0 -0 -0
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:50:00.92 +22:08:15.8: 13.00 +/- 0.03 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:50:00.92 +22:08:15.8: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
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 07.3983* 05 50 00.92 +22 08 15.8 9.3 U Ori 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,2461259.8983,9.28,0.05,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 20260807.3983 9.28CV 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 07.3983* 05 46 53.51 +23 34 48.5 6.7 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,2461259.8983,6.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260807.3983 6.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 07.3983* 05 21 07.66 +23 38 19.8 10.8 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
target,2461259.8983,10.77,0.05,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
target 20260807.3983 10.77CV 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 07.3983 2461259.8983 11.27 05:59:24.80 +22:53:59.9
186.77316 -0.40546 galactic Tau Second-epoch detections are separated by 0.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.27 Euterpe 0 -1 1 11.6 0 0
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:59:24.80 +22:53:59.9: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:59:24.80 +22:53:59.9: 15.80 +/- 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 07.3983* 05 59 24.80 +22 53 59.9 11.3 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,2461259.8983,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260807.3983 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.3983 2461259.8983 11.77 05:34:37.59 +23:29:26.4
183.31753 -4.97461 galactic Tau Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.22 Kalliope 1 1 1 12.3 -0 -0
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:34:37.59 +23:29:26.4: 15.30 +/- 0.16 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:34:37.59 +23:29:26.4: 15.48 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.37 +/- 0.13
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 07.3983* 05 34 37.59 +23 29 26.4 11.8 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,2461259.8983,11.77,0.05,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 20260807.3983 11.77CV 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 07.3983 2461259.8983 12.35 05:28:17.51 +21:43:12.9
184.01976 -7.16185 galactic Tau Second-epoch detections are separated by 2.0" and 6.0 pix
The object was found in VSX 2" ASASSN-V J052817.61+214313.9
Type: L
# Max. Min./Amp. JD0 Period
13.240 V 13.660 V
The object was not found in astcheck.
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:28:17.51 +21:43:12.9: 13.30 +/- 0.02 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:28:17.51 +21:43:12.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
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 07.3983* 05 28 17.51 +21 43 12.9 12.3 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
ASASSN-V J052817.61+214313.9,2461259.8983,12.35,0.05,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
ASASSN-V J052817.61+214313.9 20260807.3983 12.35CV 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 07.3983 2461259.8983 12.15 05:57:08.74 +24:49:54.3
184.84083 0.11096 galactic Tau Second-epoch detections are separated by 1.9" and 6.3 pix
The object was found in VSX 1" ASASSN-V J055708.65+244953.7
Type: SR
# Max. Min./Amp. JD0 Period
13.730 V 14.010 V 2458351.05530 65.134677100000
The object was not found in astcheck.
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:57:08.74 +24:49:54.3: 13.29 +/- 0.03 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:57:08.74 +24:49:54.3: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
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 07.3983* 05 57 08.74 +24 49 54.3 12.2 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
ASASSN-V J055708.65+244953.7,2461259.8983,12.15,0.05,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
ASASSN-V J055708.65+244953.7 20260807.3983 12.15CV 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 07.3983 2461259.8983 12.36 05:37:52.53 +23:35:25.4
183.63215 -4.29189 galactic Tau Second-epoch detections are separated by 1.6" and 5.8 pix
The object was found in VSX 2" ZTF J053752.42+233525.1
Type: SR
# Max. Min./Amp. JD0 Period
15.006 g Y 0.553 g 2458427.28040 130.112752900000
The object was not found in astcheck.
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:37:52.53 +23:35:25.4: 13.25 +/- 0.02 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:37:52.53 +23:35:25.4: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
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 07.3983* 05 37 52.53 +23 35 25.4 12.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J053752.42+233525.1,2461259.8983,12.36,0.05,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
ZTF J053752.42+233525.1 20260807.3983 12.36CV 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 07.3983 2461259.8983 12.14 05:48:04.30 +20:45:29.0
187.28930 -3.75933 galactic Tau Second-epoch detections are separated by 2.8" and 6.4 pix
The object was found in VSX 1" ASASSN-V J054804.19+204529.2
Type: L
# Max. Min./Amp. JD0 Period
13.530 V 13.960 V
The object was not found in astcheck.
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:48:04.30 +20:45:29.0: 13.18 +/- 0.03 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:48:04.30 +20:45:29.0: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
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 07.3983* 05 48 04.30 +20 45 29.0 12.1 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
ASASSN-V J054804.19+204529.2,2461259.8983,12.14,0.05,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
ASASSN-V J054804.19+204529.2 20260807.3983 12.14CV 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 07.3983 2461259.8983 11.05 05:36:07.54 +17:51:49.4
188.29900 -7.67206 galactic Tau Second-epoch detections are separated by 1.2" and 6.1 pix
The object was found in VSX 1" NSV 2365
Type: SRB
# Max. Min./Amp. JD0 Period
12.100 V 13.000 V 2452964.00000 50.410000000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:36:07.54 +17:51:49.4: 11.95 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:36:07.54 +17:51:49.4: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
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 07.3983* 05 36 07.54 +17 51 49.4 11.1 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
NSV 2365,2461259.8983,11.05,0.05,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
NSV 2365 20260807.3983 11.05CV 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 07.3983 2461259.8983 10.81 05:31:40.76 +16:57:37.1
188.50664 -9.05007 galactic Tau Second-epoch detections are separated by 0.7" and 6.1 pix
The object was found in VSX 1" ASAS J053141+1657.6
Type: MISC
# Max. Min./Amp. JD0 Period
8.349 Ic Y 0.448 Ic 2452707.70000 156.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:31:40.76 +16:57:37.1: 11.91 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:31:40.76 +16:57:37.1: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
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 07.3983* 05 31 40.76 +16 57 37.1 10.8 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
ASAS J053141+1657.6,2461259.8983,10.81,0.05,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
ASAS J053141+1657.6 20260807.3983 10.81CV 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 07.3983 2461259.8983 10.41 05:39:34.84 +18:52:39.1
187.86353 -6.44203 galactic Tau Second-epoch detections are separated by 0.3" and 6.1 pix
The object was found in VSX 1" V1261 Tau
Type: SRB
# Max. Min./Amp. JD0 Period
12.000 V 13.000 V 2452955.80000 123.000000000000 M5
The object was not found in astcheck.
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:39:34.84 +18:52:39.1: 11.38 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:39:34.84 +18:52:39.1: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.00
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 07.3983* 05 39 34.84 +18 52 39.1 10.4 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
V1261 Tau,2461259.8983,10.41,0.05,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
V1261 Tau 20260807.3983 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.3983 2461259.8983 10.18 05:44:42.56 +17:39:03.5
189.55396 -6.03821 galactic Tau Second-epoch detections are separated by 1.7" and 6.3 pix
The object was found in VSX 1" ASAS J054443+1739.1
Type: MISC
# Max. Min./Amp. JD0 Period
11.680 V Y 0.370 V 2452804.90000 101.750102000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:44:42.56 +17:39:03.5: 11.00 +/- 0.00 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:44:42.56 +17:39:03.5: 11.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.00
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 07.3983* 05 44 42.56 +17 39 03.5 10.2 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
ASAS J054443+1739.1,2461259.8983,10.18,0.05,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
ASAS J054443+1739.1 20260807.3983 10.18CV 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: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
First image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461259.89862045 07.08.2026 09:33:50.807 /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.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.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 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): 20170
Objects passed selection criteria: 20034
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 12556.8
Average stars matched: 12377.5 (98.5725 %)
Memory usage VmPeak: 245516 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Aug 7 04:40:33 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
First image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461259.89862045 07.08.2026 09:33:50.807 /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 99
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 20 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): 149858
Objects passed selection criteria: 149365
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 95375.5
Average stars matched: 92112.5 (96.5788 %)
Memory usage VmPeak: 550688 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Aug 7 04:41:44 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
SExtractor catalog cache: saved Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.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: 2461259.89801590
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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
Saving wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits to local_wcs_cache/
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'local_wcs_cache/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits exists and is non-empty
Saving wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits to local_wcs_cache/
'wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits' -> 'local_wcs_cache/wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits'
wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits'
wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (1st reference image)
verification OK: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:32:19.570 +21:59:57.74 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-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits (1st new image)
verification OK: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:32:27.813 +22:00:06.11 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:32:19.570 +21:59:57.74
Second-epoch image center 05:32:27.813 +22:00:06.11
Angular distance between the image centers 0.0319 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits (2nd new image)
verification OK: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:32:25.419 +21:59:58.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.570 +21:59:57.74
Second-epoch image center 05:32:25.419 +21:59:58.14
Angular distance between the image centers 0.0226 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 05:32:27.813 +22:00:06.11
Second-epoch second image center 05:32:25.419 +21:59:58.14
Angular distance between the image centers 0.00951 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.VY6FIAMncY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits &> /tmp/tmp.NXSlmhH2yP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits &> /tmp/tmp.Qr6V0c0792
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits &> /tmp/tmp.0XLWUOrC7Z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
The reference image (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat) found
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat' -> 'wcsmag.cat'
Read 22997 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3514 to 91.9479 deg, Dec +16.4790 to +27.2884 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 74.3514 to 91.9479 deg, Dec 16.4790 to 27.2884 deg
Loaded 12406 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): 8976 out of 10160 total matches.
Matched with Tycho-2 10160 out of 22997 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.969200
a=0.000000 b=1.000000 c=22.969200
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 22997 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3514 to 91.9479 deg, Dec +16.4790 to +27.2884 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 74.3514 to 91.9479 deg, Dec 16.4790 to 27.2884 deg
Loaded 12406 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): 8976 out of 10160 total matches.
Matched with Tycho-2 10160 out of 22997 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Forced-photometry filter: calibrated wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -> calib.txt_param_ref_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (aperture=6.0)
Read 20916 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3773 to 91.9061 deg, Dec +16.4876 to +27.3008 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 74.3773 to 91.9061 deg, Dec 16.4876 to 27.3008 deg
Loaded 12329 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): 8847 out of 10017 total matches.
Matched with Tycho-2 10017 out of 20916 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Forced-photometry filter: calibrated wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits -> calib.txt_param_ref_wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits (aperture=6.0)
____ 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
2.0 pix Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
2.9 pix fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
2.9 pix fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Limiting magnitude estimates:
15.3 mag. Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.2 mag. Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
12.7 mag. fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
12.7 mag. fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 10.5 (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
############ /tmp/tmp.VY6FIAMncY (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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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=2479, bad_region=0, passed=22997
Got 22997 stars (including 20487 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
util/solve_plate_with_UCAC5 got 22997 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4778 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 4714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 22997 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4778 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 22997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 22997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4713 stars left (next iteration limit 5184)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits N_match=4713 sigma_overall_arcsec=0.377 sigma_q1_arcsec=0.465 sigma_q2_arcsec=0.352 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.276 n_q1=1531 n_q2=718 n_q3=1554 n_q4=910 worst_quadrant_to_overall_ratio=1.235
The image catalog is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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.NXSlmhH2yP (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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits' -> 'wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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=2320, bad_region=0, passed=20916
Got 20916 stars (including 18570 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat
util/solve_plate_with_UCAC5 got 20916 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4782 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4716 matched stars entering correct_measured_positions(), 4717 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4716 matched stars entering correct_measured_positions(), 20916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 4783 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4714 matched stars entering correct_measured_positions(), 20916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4714 matched stars entering correct_measured_positions(), 20916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4714 stars left (next iteration limit 5187)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits N_match=4714 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.603 sigma_q2_arcsec=0.446 sigma_q3_arcsec=0.465 sigma_q4_arcsec=0.387 n_q1=1527 n_q2=718 n_q3=1564 n_q4=905 worst_quadrant_to_overall_ratio=1.251
The image catalog is written to wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits -region wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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.Qr6V0c0792 (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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.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=163, bad_region=0, passed=3255
Got 3255 stars (including 3091 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 3255 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 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 531 to 589 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 2965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2925 matched stars entering correct_measured_positions(), 2915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2925 matched stars entering correct_measured_positions(), 3238 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 531 to 589 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 2965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2927 matched stars entering correct_measured_positions(), 3238 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 2927 matched stars entering correct_measured_positions(), 3238 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 2927 stars left (next iteration limit 3217)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2927 robust_rms=7.698 arcsec worst_quadrant_rms=9.436 arcsec
SIP_REFIT: SIP order 3 trial: matched=2927 robust_rms=0.643 arcsec worst_quadrant_rms=0.721 arcsec
SIP_REFIT: SIP order 5 trial: matched=2927 robust_rms=0.475 arcsec worst_quadrant_rms=0.548 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2927 robust_rms_before=1.453 arcsec robust_rms_before_corrected=0.536 arcsec robust_rms_after=0.475 arcsec worst_quadrant_rms_before=0.632 worst_quadrant_rms_after=0.548
verification OK: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
verification OK: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
Image size: 945.4'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:32:27.917 +22:00:04.56 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3255 stars ###
'wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/correct_sextractor_wcs_catalog_usingxy2sky1447909.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.453 -> 0.475 arcsec)
WCS_QUALITY_DIAG: file=fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits N_match=2927 sigma_overall_arcsec=0.502 sigma_q1_arcsec=0.494 sigma_q2_arcsec=0.628 sigma_q3_arcsec=0.399 sigma_q4_arcsec=0.532 n_q1=750 n_q2=522 n_q3=677 n_q4=978 worst_quadrant_to_overall_ratio=1.253
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits -region wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.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.0XLWUOrC7Z (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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.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=159, bad_region=0, passed=3345
Got 3345 stars (including 3184 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat
util/solve_plate_with_UCAC5 got 3345 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 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 531 to 589 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 3056 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3019 matched stars entering correct_measured_positions(), 3017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3019 matched stars entering correct_measured_positions(), 3337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 531 to 589 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 3057 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3017 matched stars entering correct_measured_positions(), 3337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 3017 matched stars entering correct_measured_positions(), 3337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 3017 stars left (next iteration limit 3320)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3017 robust_rms=7.857 arcsec worst_quadrant_rms=9.060 arcsec
SIP_REFIT: SIP order 3 trial: matched=3017 robust_rms=0.631 arcsec worst_quadrant_rms=0.732 arcsec
SIP_REFIT: SIP order 5 trial: matched=3017 robust_rms=0.461 arcsec worst_quadrant_rms=0.515 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3017 robust_rms_before=1.511 arcsec robust_rms_before_corrected=0.555 arcsec robust_rms_after=0.461 arcsec worst_quadrant_rms_before=0.644 worst_quadrant_rms_after=0.515
verification OK: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
verification OK: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Image size: 945.3'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:32:25.527 +21:59:56.49 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3345 stars ###
'wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/correct_sextractor_wcs_catalog_usingxy2sky1447807.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.511 -> 0.461 arcsec)
WCS_QUALITY_DIAG: file=fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits N_match=3017 sigma_overall_arcsec=0.488 sigma_q1_arcsec=0.483 sigma_q2_arcsec=0.568 sigma_q3_arcsec=0.435 sigma_q4_arcsec=0.479 n_q1=754 n_q2=559 n_q3=693 n_q4=1011 worst_quadrant_to_overall_ratio=1.164
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits -region wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits sigma_overall=0.377 worst_q_ratio=1.235
ref2=Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits sigma_overall=0.482 worst_q_ratio=1.251
new1=fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits sigma_overall=0.502 worst_q_ratio=1.253
new2=fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits sigma_overall=0.488 worst_q_ratio=1.164
reference average sigma_overall=0.4295 worst_q_ratio=1.243
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378_astrometric_residuals.png (4713 matched stars from wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035_astrometric_residuals.png (4714 matched stars from wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410_astrometric_residuals.png (2927 matched stars from wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411_astrometric_residuals.png (3017 matched stars from wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits'
Preparing the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:50:00.92 +22:08:15.8: 13.00 +/- 0.03 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:50:00.92 +22:08:15.8: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter KEPT candidate at 05:50:00.92 +22:08:15.8: ref_mag=13.00 +/- 0.02 new_mean_mag=9.2760 delta=3.73 (need > 0.90)
Adding exclusion_list_local.txt__out10236.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 30668_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 30668_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 30705_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 30705_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 07601_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 07601_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:18:58.83 +23:30:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01239_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 01239_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:33:49.74 +26:38:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10236_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 10236_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 19272_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 19272_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:46:56.47 +17:54:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14186_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 14186_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:55:48.99 +20:10:31.0 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 16s
Prepared the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:50:00.92 +22:08:15.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
SExtractor catalog cache: saved Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Creating symlink local_wcs_cache/wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits exists and is non-empty
wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits exists and is non-empty
wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (1st reference image)
verification OK: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:32:19.570 +21:59:57.74 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-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits (1st new image)
verification OK: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:32:27.813 +22:00:06.11 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:32:19.570 +21:59:57.74
Second-epoch image center 05:32:27.813 +22:00:06.11
Angular distance between the image centers 0.0319 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits (2nd new image)
verification OK: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:32:25.419 +21:59:58.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.570 +21:59:57.74
Second-epoch image center 05:32:25.419 +21:59:58.14
Angular distance between the image centers 0.0226 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 05:32:27.813 +22:00:06.11
Second-epoch second image center 05:32:25.419 +21:59:58.14
Angular distance between the image centers 0.00951 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.xy7IRYQDl1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits &> /tmp/tmp.hihYUBgsPd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits &> /tmp/tmp.QJdgfFFDG3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits &> /tmp/tmp.MqLHLGYotf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
The reference image (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat) found
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat' -> 'wcsmag.cat'
Read 167968 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3408 to 91.9478 deg, Dec +16.4791 to +27.2941 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 74.3408 to 91.9478 deg, Dec 16.4791 to 27.2941 deg
Loaded 12414 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): 7145 out of 10502 total matches.
Matched with Tycho-2 10502 out of 167968 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.825500
a=0.000000 b=1.000000 c=22.825500
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.51
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 167968 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3408 to 91.9478 deg, Dec +16.4791 to +27.2941 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 74.3408 to 91.9478 deg, Dec 16.4791 to 27.2941 deg
Loaded 12414 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): 7145 out of 10502 total matches.
Matched with Tycho-2 10502 out of 167968 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Forced-photometry filter: calibrated wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -> calib.txt_param_ref_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (aperture=4.5)
Read 163013 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3370 to 91.9475 deg, Dec +16.4845 to +27.3051 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 74.3370 to 91.9475 deg, Dec 16.4845 to 27.3051 deg
Loaded 12419 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): 7184 out of 10475 total matches.
Matched with Tycho-2 10475 out of 163013 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Forced-photometry filter: calibrated wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits -> calib.txt_param_ref_wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 96 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
1.8 pix Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
2.7 pix fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
2.7 pix fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Limiting magnitude estimates:
15.5 mag. Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.4 mag. Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
13.1 mag. fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
13.1 mag. fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.7 (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.xy7IRYQDl1 (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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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=28, blended=21684, bad_region=13, passed=167940
Got 167940 stars (including 145983 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
util/solve_plate_with_UCAC5 got 167940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4760 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4716 matched stars entering correct_measured_positions(), 4716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4716 matched stars entering correct_measured_positions(), 167940 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4760 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4716 matched stars entering correct_measured_positions(), 167940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4716 matched stars entering correct_measured_positions(), 167940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4716 stars left (next iteration limit 5187)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits N_match=4716 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.446 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.335 sigma_q4_arcsec=0.278 n_q1=1463 n_q2=774 n_q3=1520 n_q4=959 worst_quadrant_to_overall_ratio=1.232
The image catalog is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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.hihYUBgsPd (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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits' -> 'wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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=51, blended=20219, bad_region=0, passed=162962
Got 162962 stars (including 142457 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat
util/solve_plate_with_UCAC5 got 162962 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4758 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4712 matched stars entering correct_measured_positions(), 4712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4712 matched stars entering correct_measured_positions(), 162962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 4759 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4711 matched stars entering correct_measured_positions(), 162962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4711 matched stars entering correct_measured_positions(), 162962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4711 stars left (next iteration limit 5183)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits N_match=4711 sigma_overall_arcsec=0.470 sigma_q1_arcsec=0.591 sigma_q2_arcsec=0.447 sigma_q3_arcsec=0.454 sigma_q4_arcsec=0.378 n_q1=1445 n_q2=753 n_q3=1535 n_q4=978 worst_quadrant_to_overall_ratio=1.258
The image catalog is written to wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits -region wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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.QJdgfFFDG3 (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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.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=663, bad_region=0, passed=26100
Got 26100 stars (including 25402 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 26100 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 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 4780 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4710 matched stars entering correct_measured_positions(), 4708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4710 matched stars entering correct_measured_positions(), 26059 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 4781 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 26060 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 26060 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4713 stars left (next iteration limit 5181)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits N_match=4713 sigma_overall_arcsec=0.525 sigma_q1_arcsec=0.558 sigma_q2_arcsec=0.612 sigma_q3_arcsec=0.421 sigma_q4_arcsec=0.500 n_q1=1194 n_q2=853 n_q3=1160 n_q4=1506 worst_quadrant_to_overall_ratio=1.166
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits -region wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.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.MqLHLGYotf (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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.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=1, no_mag_err=0, low_SNR=1, blended=683, bad_region=1, passed=26618
Got 26618 stars (including 25895 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat
util/solve_plate_with_UCAC5 got 26618 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 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 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4774 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4703 matched stars entering correct_measured_positions(), 4702 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4703 matched stars entering correct_measured_positions(), 26581 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4775 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 26582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 26582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4705 stars left (next iteration limit 5173)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits N_match=4705 sigma_overall_arcsec=0.539 sigma_q1_arcsec=0.543 sigma_q2_arcsec=0.619 sigma_q3_arcsec=0.448 sigma_q4_arcsec=0.497 n_q1=1184 n_q2=875 n_q3=1137 n_q4=1509 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits -region wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.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-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-32-58_20.00sec_-0.00C_LIGHTs_0410.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.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_2026-08-07_CI_Tau-04-Q1b1x1_043555_TTUQ1b1x1_1365590_HPH2KxEY/wcs_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411.fits
Preparing the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:59:24.80 +22:53:59.9: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:11:57.37 +24:41:59.6: 12.06 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:09:07.91 +21:52:54.9: 12.21 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:34:37.59 +23:29:26.4: 15.30 +/- 0.16 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:32:49.68 +26:44:16.9: 12.21 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:09:07.91 +21:52:54.9: 12.21 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:59:24.80 +22:53:59.9: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:11:57.37 +24:41:59.6: 12.08 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:34:37.59 +23:29:26.4: 15.48 +/- 0.20 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry reference-image weighted average: 15.37 +/- 0.13
Forced photometry filter REJECTED candidate at 05:09:07.91 +21:52:54.9: ref_mag=12.21 +/- 0.01 new_mean_mag=12.3759 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:11:57.37 +24:41:59.6: ref_mag=12.07 +/- 0.01 new_mean_mag=12.1406 delta=-0.07 (need > 0.90)
Forced photometry filter KEPT candidate at 05:34:37.59 +23:29:26.4: ref_mag=15.37 +/- 0.13 new_mean_mag=11.7640 delta=3.61 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:32:49.68 +26:44:16.9: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry filter REJECTED candidate at 05:32:49.68 +26:44:16.9: ref_mag=12.21 +/- 0.01 new_mean_mag=12.1576 delta=0.05 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:42:54.51 +21:13:26.9: 12.96 +/- 0.02 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:57:08.74 +24:49:54.3: 13.29 +/- 0.03 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:28:17.51 +21:43:12.9: 13.30 +/- 0.02 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:42:54.51 +21:13:26.9: 12.93 +/- 0.02 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:37:52.53 +23:35:25.4: 13.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.01
Forced photometry filter REJECTED candidate at 05:42:54.51 +21:13:26.9: ref_mag=12.95 +/- 0.01 new_mean_mag=12.1615 delta=0.79 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:57:08.74 +24:49:54.3: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry filter KEPT candidate at 05:57:08.74 +24:49:54.3: ref_mag=13.31 +/- 0.03 new_mean_mag=12.1589 delta=1.15 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:28:17.51 +21:43:12.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 05:28:17.51 +21:43:12.9: ref_mag=13.26 +/- 0.02 new_mean_mag=12.3482 delta=0.91 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:37:52.53 +23:35:25.4: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 05:37:52.53 +23:35:25.4: ref_mag=13.28 +/- 0.02 new_mean_mag=12.3178 delta=0.96 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:48:04.30 +20:45:29.0: 13.18 +/- 0.03 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:48:04.30 +20:45:29.0: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 05:48:04.30 +20:45:29.0: ref_mag=13.10 +/- 0.02 new_mean_mag=12.1310 delta=0.97 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:30:46.19 +22:50:44.5: 13.12 +/- 0.02 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:30:46.19 +22:50:44.5: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter REJECTED candidate at 05:30:46.19 +22:50:44.5: ref_mag=13.21 +/- 0.02 new_mean_mag=12.3178 delta=0.90 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:36:07.54 +17:51:49.4: 11.95 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:31:40.76 +16:57:37.1: 11.91 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:36:07.54 +17:51:49.4: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Forced photometry filter KEPT candidate at 05:36:07.54 +17:51:49.4: ref_mag=11.97 +/- 0.01 new_mean_mag=11.0526 delta=0.92 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:31:40.76 +16:57:37.1: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter KEPT candidate at 05:31:40.76 +16:57:37.1: ref_mag=11.90 +/- 0.01 new_mean_mag=10.8064 delta=1.09 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:39:34.84 +18:52:39.1: 11.38 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:44:42.56 +17:39:03.5: 11.00 +/- 0.00 detection
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:39:34.84 +18:52:39.1: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.00
Forced photometry filter KEPT candidate at 05:39:34.84 +18:52:39.1: ref_mag=11.37 +/- 0.00 new_mean_mag=10.4121 delta=0.96 (need > 0.90)
Forced photometry on wcs_Tau-04-Q1b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:44:42.56 +17:39:03.5: 11.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.00
Forced photometry filter KEPT candidate at 05:44:42.56 +17:39:03.5: ref_mag=11.12 +/- 0.00 new_mean_mag=10.1690 delta=0.95 (need > 0.90)
Adding exclusion_list_local.txt__out101559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86301.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
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: 7s
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Considering the candidate 190568_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190568_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
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Considering the candidate 190569_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190569_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
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Considering the candidate 190572_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 190572_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 190582_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190582_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:43:29.67 +16:41:53.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 190611_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 190611_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 190613_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190613_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:07:58.93 +26:19:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190705_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 190705_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 190720_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 190720_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 190734_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190734_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:05:06.86 +23:48:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190740_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190740_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:05:45.96 +26:25:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190742_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190742_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:41:56.13 +22:38:55.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190749_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190749_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:32:16.93 +17:02:05.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190767_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190767_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
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Considering the candidate 190781_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190781_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:35:02.43 +26:58:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190794_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190794_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:30:50.72 +22:27:25.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190802_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190802_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:39:10.62 +23:20:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190814_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190814_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:05:41.72 +23:02:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190818_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190818_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:10:01.81 +26:45:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190852_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190852_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:19:43.94 +26:10:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190872_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 190872_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:39:54.80 +23:41:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57016_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 57016_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:18:58.85 +23:30:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58778_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 58778_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:33:52.73 +23:22:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33497_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 33497_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:54:08.14 +24:51:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157320_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 157320_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:19:47.19 +17:10:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82933_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 82933_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:53:50.65 +21:45:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145353_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 145353_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:21:12.62 +19:30:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104863_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 104863_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:32:33.01 +20:37:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76761_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 76761_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:23:57.87 +22:13:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59493_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 59493_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:48:36.78 +23:10:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127266_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 127266_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:02:18.60 +18:20:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57765_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 57765_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:22:03.19 +23:24:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93856_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 93856_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
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Considering the candidate 86301_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 86301_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 45018_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 45018_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:48:29.21 +24:10:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32915_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 32915_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 67949_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 67949_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:53:46.79 +22:35:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54813_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 54813_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 19093_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 19093_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 06:00:43.55 +25:40:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110271_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 110271_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:24:37.35 +20:19:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101559_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 101559_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 66461_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 66461_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
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Considering the candidate 81365_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 81365_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:54:40.87 +21:49:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167486_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 167486_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:30:33.67 +17:49:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142657_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 142657_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:36:37.77 +19:21:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86369_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 86369_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:56:16.72 +21:31:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114972_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 114972_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:16:28.87 +20:02:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143505_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 143505_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:37:40.87 +19:24:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166618_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 166618_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:45:25.38 +17:43:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71919_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 71919_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:32:15.27 +22:31:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76504_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 76504_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:50:00.93 +22:08:15.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 108934_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 108934_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:30:18.30 +20:22:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120168_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 120168_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:46:56.50 +17:54:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09594_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 09594_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:48:40.01 +26:28:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18962_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 18962_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 06:06:18.00 +25:36:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109495_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 109495_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:34:26.43 +20:22:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27363_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 27363_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:50:00.54 +25:17:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128442_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 128442_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:44:37.89 +18:24:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145044_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 145044_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:51:01.72 +19:24:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43431_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 43431_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:52:58.81 +24:14:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118951_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 118951_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:34:41.17 +17:53:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126031_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 126031_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:18:00.35 +18:21:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118724_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 118724_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 122051_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 122051_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
Rejecting candidate due to large distance (35.1") between the two second-epoch detections
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Considering the candidate 153854_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 153854_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 80276_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 80276_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:56:11.20 +21:51:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25835_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 25835_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:49:48.85 +25:25:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49183_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 49183_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:53:41.41 +23:51:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08476_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 08476_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:33:49.73 +26:38:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135311_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 135311_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 106761_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 106761_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:39:15.60 +20:28:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165516_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
Preparing report for the candidate 165516_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
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Considering the candidate 111854_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 111854_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:55:49.00 +20:10:31.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53615_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 53615_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:19:46.63 +23:40:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84793_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 84793_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:27:38.21 +21:56:10.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 108697_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 108697_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:33:38.79 +20:28:28.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 96330_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 96330_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:37:38.52 +21:08:30.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 70278_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 70278_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:42:03.88 +22:39:35.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 49964_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 49964_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:35:27.11 +24:02:18.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 66296_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 66296_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:57:07.25 +22:50:19.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 105095_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 105095_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:45:39.29 +20:41:42.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 117978_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 117978_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:32:12.71 +18:35:43.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129379_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 129379_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:33:31.59 +18:32:27.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101378_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 101378_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:48:22.29 +20:52:09.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 18851_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 18851_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:39:44.12 +25:53:46.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 120138_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 120138_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:27:10.13 +17:57:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 163269_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 163269_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:41:22.57 +17:31:20.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 39648_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 39648_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:49:00.79 +24:33:59.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116845_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 116845_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:52:23.38 +19:52:04.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 157917_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 157917_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:28:01.67 +17:14:21.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 160317_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 160317_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:24:26.05 +17:23:03.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 155021_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 155021_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:32:14.27 +17:03:26.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 155271_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 155271_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:37:03.72 +17:02:25.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 110647_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 110647_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:54:22.42 +20:16:31.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14039_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 14039_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 05:57:59.57 +25:57:13.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 58326_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 58326_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
**** FOUND 06:04:07.09 +23:15:44.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 166587_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411
The candidate 166587_fd_Tau-04-Q1b1x1_2026-08-07_04-33-50_20.00sec_-0.00C_LIGHTs_0411 did not pass the final checks
