This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 10 12.3456 2461325.8456 13.20 04:36:58.35 +25:26:36.2
173.86918 -14.42041 galactic Tau Second-epoch detections are separated by 0.7" and 11.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.344 Desiderata -0 1 1 13.2 0 0
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:36:58.35 +25:26:36.2: 16.37 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:36:58.35 +25:26:36.2: 16.26 +/- 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 10 12.3456* 04 36 58.35 +25 26 36.2 13.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461325.8456,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.3456 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.3456 2461325.8456 13.62 04:33:09.76 +25:50:50.9
172.97614 -14.81259 galactic Tau Second-epoch detections are separated by 0.0" and 11.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.112 Iphigenia -0 1 1 13.5 0 0
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:33:09.76 +25:50:50.9: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:33:09.76 +25:50:50.9: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 12.3456* 04 33 09.76 +25 50 50.9 13.6 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,2461325.8456,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.3456 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.3456 2461325.8456 14.41 04:49:54.80 +23:17:11.9
177.50623 -13.48437 galactic Tau Second-epoch detections are separated by 0.6" and 11.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1219 Britta -1 1 1 14.7 0 0
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:49:54.80 +23:17:11.9: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:49:54.80 +23:17:11.9: 16.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 12.3456* 04 49 54.80 +23 17 11.9 14.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461325.8456,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.3456 14.41CV 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 10 12.3456 2461325.8456 14.37 04:53:53.99 +21:33:39.3
179.49257 -13.80175 galactic Tau Second-epoch detections are separated by 1.5" and 11.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.940 Kordula 0 0 0 14.6 0 0
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:53:53.99 +21:33:39.3: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:53:53.99 +21:33:39.3: 16.18 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 12.3456* 04 53 53.99 +21 33 39.3 14.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461325.8456,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.3456 14.37CV 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 10 12.3456 2461325.8456 14.86 04:43:54.65 +20:28:55.1
178.90791 -16.30752 galactic Tau Second-epoch detections are separated by 1.1" and 11.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.311 Claudia -0 -2 2 14.9 0 0
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:43:54.65 +20:28:55.1: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:43:54.65 +20:28:55.1: 16.20 +/- 0.36 detection
Forced photometry reference-image weighted average: 16.20 +/- 0.36
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 10 12.3456* 04 43 54.65 +20 28 55.1 14.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461325.8456,14.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.3456 14.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461325.84600612 12.10.2026 08:18:04.929 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 10539
Objects passed selection criteria: 10502
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 8041
Average stars matched: 7411.75 (92.1745 %)
Memory usage VmPeak: 235552 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 12 03:37:13 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461325.84600612 12.10.2026 08:18:04.929 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 131
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.93
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: 38 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): 77413
Objects passed selection criteria: 77214
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 60531.2
Average stars matched: 55689 (92.0004 %)
Memory usage VmPeak: 288932 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 12 03:38:44 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/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461325.84527300
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits exists and is non-empty
wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (1st reference image)
verification OK: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:56.045 +21:59:37.33 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits (1st new image)
verification OK: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:36:55.837 +21:59:56.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:36:56.045 +21:59:37.33
Second-epoch image center 04:36:55.837 +21:59:56.91
Angular distance between the image centers 0.0055 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits (2nd new image)
verification OK: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:36:58.985 +22:00:46.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:36:56.045 +21:59:37.33
Second-epoch image center 04:36:58.985 +22:00:46.91
Angular distance between the image centers 0.0224 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:36:55.837 +21:59:56.91
Second-epoch second image center 04:36:58.985 +22:00:46.91
Angular distance between the image centers 0.01846 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.f4bVoUQRDp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.KwRQBGgQn1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits &> /tmp/tmp.m9CuZhUyg6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits &> /tmp/tmp.f09z8BFe4k
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
The reference image (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat) found
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat' -> 'wcsmag.cat'
Read 11927 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5112 to 78.0902 deg, Dec +16.4856 to +27.2829 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 60.5112 to 78.0902 deg, Dec 16.4856 to 27.2829 deg
Loaded 5180 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3947 out of 4318 total matches.
Matched with Tycho-2 4318 out of 11927 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.991000
a=0.000000 b=1.000000 c=22.991000
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.75
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.75
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11927 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5112 to 78.0902 deg, Dec +16.4856 to +27.2829 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 60.5112 to 78.0902 deg, Dec 16.4856 to 27.2829 deg
Loaded 5180 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3947 out of 4318 total matches.
Matched with Tycho-2 4318 out of 11927 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Forced-photometry filter: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -> calib.txt_param_ref_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (aperture=5.9)
Read 11076 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5314 to 78.0905 deg, Dec +16.4856 to +27.2796 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 60.5314 to 78.0905 deg, Dec 16.4856 to 27.2796 deg
Loaded 5169 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3956 out of 4300 total matches.
Matched with Tycho-2 4300 out of 11076 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Forced-photometry filter: calibrated wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits -> calib.txt_param_ref_wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
2.1 pix Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
2.4 pix fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
2.4 pix fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Limiting magnitude estimates:
15.7 mag. Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.6 mag. Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
15.5 mag. fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
15.5 mag. fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.f4bVoUQRDp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=967, bad_region=2517, passed=11927
Got 11927 stars (including 8622 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
util/solve_plate_with_UCAC5 got 11927 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4850 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 4820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 9924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4851 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 9924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 9924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4820 stars left (next iteration limit 5302)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits N_match=4820 sigma_overall_arcsec=0.311 sigma_q1_arcsec=0.399 sigma_q2_arcsec=0.319 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.247 n_q1=1641 n_q2=611 n_q3=1816 n_q4=752 worst_quadrant_to_overall_ratio=1.284
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.KwRQBGgQn1 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=897, bad_region=2444, passed=11076
Got 11076 stars (including 7922 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat
util/solve_plate_with_UCAC5 got 11076 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4847 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 4817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 9127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 4848 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 9127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 9127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4818 stars left (next iteration limit 5298)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits N_match=4818 sigma_overall_arcsec=0.366 sigma_q1_arcsec=0.456 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.331 sigma_q4_arcsec=0.291 n_q1=1645 n_q2=622 n_q3=1785 n_q4=766 worst_quadrant_to_overall_ratio=1.245
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.m9CuZhUyg6 (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_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.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_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=691, bad_region=3217, passed=10311
Got 10311 stars (including 6588 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat
util/solve_plate_with_UCAC5 got 10311 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 7719 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 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 7719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 7719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4869 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4869 robust_rms=8.060 arcsec worst_region_rms=13.030 arcsec outer_annulus_rms=13.030 arcsec
SIP_REFIT: SIP order 3 trial: matched=4869 robust_rms=0.511 arcsec worst_region_rms=0.733 arcsec outer_annulus_rms=0.733 arcsec
SIP_REFIT: SIP order 5 trial: matched=4869 robust_rms=0.392 arcsec worst_region_rms=0.490 arcsec outer_annulus_rms=0.490 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4869 robust_rms_before=1.135 arcsec robust_rms_before_corrected=0.420 arcsec robust_rms_after=0.392 arcsec worst_region_rms_before=0.522 worst_region_rms_after=0.490 outer_annulus_rms_before=1.231 outer_annulus_rms_after=0.490
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.522 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits worst_region_rms_kept=0.522 arcsec robust_rms_kept=0.420 arcsec matched=4869
WCS_QUALITY_DIAG: file=fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits N_match=4869 sigma_overall_arcsec=0.441 sigma_q1_arcsec=0.368 sigma_q2_arcsec=0.437 sigma_q3_arcsec=0.455 sigma_q4_arcsec=0.490 n_q1=1431 n_q2=1145 n_q3=1483 n_q4=810 worst_quadrant_to_overall_ratio=1.112
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits -region wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.f09z8BFe4k (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_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.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_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=692, bad_region=3213, passed=10413
Got 10413 stars (including 6692 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat
util/solve_plate_with_UCAC5 got 10413 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 4867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 7832 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 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 7832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 7832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4868 stars left (next iteration limit 5353)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4868 robust_rms=8.077 arcsec worst_region_rms=13.071 arcsec outer_annulus_rms=13.071 arcsec
SIP_REFIT: SIP order 3 trial: matched=4868 robust_rms=0.519 arcsec worst_region_rms=0.782 arcsec outer_annulus_rms=0.782 arcsec
SIP_REFIT: SIP order 5 trial: matched=4868 robust_rms=0.395 arcsec worst_region_rms=0.542 arcsec outer_annulus_rms=0.542 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4868 robust_rms_before=1.128 arcsec robust_rms_before_corrected=0.425 arcsec robust_rms_after=0.395 arcsec worst_region_rms_before=0.565 worst_region_rms_after=0.542 outer_annulus_rms_before=1.265 outer_annulus_rms_after=0.542
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.565 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits worst_region_rms_kept=0.565 arcsec robust_rms_kept=0.425 arcsec matched=4868
WCS_QUALITY_DIAG: file=fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits N_match=4868 sigma_overall_arcsec=0.442 sigma_q1_arcsec=0.382 sigma_q2_arcsec=0.455 sigma_q3_arcsec=0.469 sigma_q4_arcsec=0.466 n_q1=1435 n_q2=1132 n_q3=1483 n_q4=818 worst_quadrant_to_overall_ratio=1.061
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits -region wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits to local_wcs_cache/
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
Saving the final (post-refit) wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits to local_wcs_cache/
'wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits' -> 'local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits'
Saving the final (post-refit) wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits'
Saving the final (post-refit) wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits sigma_overall=0.311 worst_q_ratio=1.284
ref2=Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits sigma_overall=0.366 worst_q_ratio=1.245
new1=fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits sigma_overall=0.441 worst_q_ratio=1.112
new2=fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits sigma_overall=0.442 worst_q_ratio=1.061
reference average sigma_overall=0.3385 worst_q_ratio=1.2645
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161_astrometric_residuals.png (4820 matched stars from wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202_astrometric_residuals.png (4818 matched stars from wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460_astrometric_residuals.png (4869 matched stars from wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461_astrometric_residuals.png (4868 matched stars from wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.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-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits'
Saving fully-calibrated image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits'
Preparing the HTML report for the field Tau-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:37:06.50 +21:14:33.2: 12.53 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:35:44.28 +21:57:42.9: 12.42 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:24:24.00 +17:53:04.2: 12.51 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:39:26.22 +22:23:30.3: 12.56 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:24:24.00 +17:53:04.2: 12.44 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:37:06.50 +21:14:33.2: 12.53 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:39:26.22 +22:23:30.3: 12.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter REJECTED candidate at 04:24:24.00 +17:53:04.2: ref_mag=12.48 +/- 0.01 new_mean_mag=12.4421 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter REJECTED candidate at 04:37:06.50 +21:14:33.2: ref_mag=12.53 +/- 0.01 new_mean_mag=12.5048 delta=0.03 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:35:44.28 +21:57:42.9: 12.42 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 04:39:26.22 +22:23:30.3: ref_mag=12.57 +/- 0.01 new_mean_mag=12.5567 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter REJECTED candidate at 04:35:44.28 +21:57:42.9: ref_mag=12.42 +/- 0.01 new_mean_mag=12.3699 delta=0.05 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 21848_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 21848_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 21956_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 21956_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22017_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 22017_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 22058_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 22058_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 07981_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 07981_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:21:25.56 +20:15:59.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Tau-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Creating symlink local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits exists and is non-empty
wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (1st reference image)
verification OK: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:56.045 +21:59:37.33 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits (1st new image)
verification OK: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:36:55.837 +21:59:56.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:36:56.045 +21:59:37.33
Second-epoch image center 04:36:55.837 +21:59:56.91
Angular distance between the image centers 0.0055 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits (2nd new image)
verification OK: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:36:58.985 +22:00:46.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:36:56.045 +21:59:37.33
Second-epoch image center 04:36:58.985 +22:00:46.91
Angular distance between the image centers 0.0224 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:36:55.837 +21:59:56.91
Second-epoch second image center 04:36:58.985 +22:00:46.91
Angular distance between the image centers 0.01846 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.7ET922hQUC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.SH0vjr60Sm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits &> /tmp/tmp.6JoM9kQTWg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits &> /tmp/tmp.vAJE9XBTbq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
The reference image (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat) found
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat' -> 'wcsmag.cat'
Read 86341 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5065 to 78.1101 deg, Dec +16.4673 to +27.2853 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 60.5065 to 78.1101 deg, Dec 16.4673 to 27.2853 deg
Loaded 5193 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3472 out of 4349 total matches.
Matched with Tycho-2 4349 out of 86341 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.845600
a=0.000000 b=1.000000 c=22.845600
From vast_summary.log: estimated ref. image limiting mag.: -6.93
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.92
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.92
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 86341 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5065 to 78.1101 deg, Dec +16.4673 to +27.2853 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 60.5065 to 78.1101 deg, Dec 16.4673 to 27.2853 deg
Loaded 5193 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3472 out of 4349 total matches.
Matched with Tycho-2 4349 out of 86341 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Forced-photometry filter: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -> calib.txt_param_ref_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (aperture=4.4)
Read 80651 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5064 to 78.1103 deg, Dec +16.4671 to +27.2945 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 60.5064 to 78.1103 deg, Dec 16.4671 to 27.2945 deg
Loaded 5197 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3489 out of 4349 total matches.
Matched with Tycho-2 4349 out of 80651 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Forced-photometry filter: calibrated wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits -> calib.txt_param_ref_wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 105 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
1.9 pix Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
2.2 pix fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
2.2 pix fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Limiting magnitude estimates:
15.9 mag. Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.8 mag. Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
15.7 mag. fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
15.7 mag. fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
All-image limiting magnitude estimate: 15.7 (SNR ) 14.9 (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.7ET922hQUC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=6242, bad_region=13891, passed=86324
Got 86324 stars (including 66886 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
util/solve_plate_with_UCAC5 got 86324 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 4848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 75480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 75480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 75480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4848 stars left (next iteration limit 5332)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits N_match=4848 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.305 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.248 n_q1=1602 n_q2=612 n_q3=1848 n_q4=786 worst_quadrant_to_overall_ratio=1.250
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.SH0vjr60Sm (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=5759, bad_region=13221, passed=80633
Got 80633 stars (including 62313 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat
util/solve_plate_with_UCAC5 got 80633 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4859 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 4845 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 70302 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 4860 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 70302 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 70302 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4844 stars left (next iteration limit 5329)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits N_match=4844 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.443 sigma_q2_arcsec=0.332 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.285 n_q1=1583 n_q2=633 n_q3=1821 n_q4=807 worst_quadrant_to_overall_ratio=1.257
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.6JoM9kQTWg (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_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.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_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=4409, bad_region=16091, passed=68118
Got 68118 stars (including 49164 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat
util/solve_plate_with_UCAC5 got 68118 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 4874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 55946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 55946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 55934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4873 stars left (next iteration limit 5361)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4873 robust_rms=8.068 arcsec worst_region_rms=12.963 arcsec outer_annulus_rms=12.963 arcsec
SIP_REFIT: SIP order 3 trial: matched=4873 robust_rms=0.510 arcsec worst_region_rms=0.783 arcsec outer_annulus_rms=0.783 arcsec
SIP_REFIT: SIP order 5 trial: matched=4873 robust_rms=0.393 arcsec worst_region_rms=0.501 arcsec outer_annulus_rms=0.501 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4873 robust_rms_before=1.122 arcsec robust_rms_before_corrected=0.410 arcsec robust_rms_after=0.393 arcsec worst_region_rms_before=0.513 worst_region_rms_after=0.501 outer_annulus_rms_before=1.212 outer_annulus_rms_after=0.501
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.513 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits worst_region_rms_kept=0.513 arcsec robust_rms_kept=0.410 arcsec matched=4873
WCS_QUALITY_DIAG: file=fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits N_match=4873 sigma_overall_arcsec=0.432 sigma_q1_arcsec=0.366 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.456 sigma_q4_arcsec=0.484 n_q1=1456 n_q2=1114 n_q3=1479 n_q4=824 worst_quadrant_to_overall_ratio=1.119
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits -region wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.vAJE9XBTbq (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_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.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_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=4355, bad_region=15919, passed=67633
Got 67633 stars (including 48854 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat
util/solve_plate_with_UCAC5 got 67633 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 4879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 55544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 55544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4878 matched stars entering correct_measured_positions(), 55537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4878 stars left (next iteration limit 5366)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4878 robust_rms=8.104 arcsec worst_region_rms=12.757 arcsec outer_annulus_rms=12.757 arcsec
SIP_REFIT: SIP order 3 trial: matched=4878 robust_rms=0.520 arcsec worst_region_rms=0.829 arcsec outer_annulus_rms=0.829 arcsec
SIP_REFIT: SIP order 5 trial: matched=4878 robust_rms=0.398 arcsec worst_region_rms=0.540 arcsec outer_annulus_rms=0.540 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4878 robust_rms_before=1.120 arcsec robust_rms_before_corrected=0.414 arcsec robust_rms_after=0.398 arcsec worst_region_rms_before=0.571 worst_region_rms_after=0.540 outer_annulus_rms_before=1.253 outer_annulus_rms_after=0.540
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.571 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits worst_region_rms_kept=0.571 arcsec robust_rms_kept=0.414 arcsec matched=4878
WCS_QUALITY_DIAG: file=fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits N_match=4878 sigma_overall_arcsec=0.427 sigma_q1_arcsec=0.370 sigma_q2_arcsec=0.431 sigma_q3_arcsec=0.462 sigma_q4_arcsec=0.451 n_q1=1456 n_q2=1108 n_q3=1490 n_q4=824 worst_quadrant_to_overall_ratio=1.081
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits -region wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.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_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-17-01_20.00sec_-0.00C_LIGHT_0460.fits
Saving fully-calibrated image wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.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_2026-10-12_CI_Tau-03-Q2b1x1_033444_TTUQ2b1x1_244910_9x6XA6O3/wcs_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461.fits
Preparing the HTML report for the field Tau-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:25:14.52 +21:32:48.1: 15.22 +/- 0.12 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:23:43.69 +23:23:32.4: 15.34 +/- 0.14 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:42:54.42 +20:21:12.8: 15.05 +/- 0.10 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:37:54.77 +20:14:05.6: 14.91 +/- 0.09 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:46:37.83 +22:25:10.0: 14.95 +/- 0.11 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:32:53.02 +19:13:37.1: 14.88 +/- 0.09 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:52:16.35 +24:48:06.8: 15.12 +/- 0.12 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:50:59.40 +24:14:00.1: 15.07 +/- 0.12 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:46:42.60 +23:47:52.8: 15.18 +/- 0.13 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:28:28.10 +24:16:21.3: 15.14 +/- 0.12 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:46:42.60 +23:47:52.8: 15.54 +/- 0.18 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:23:43.69 +23:23:32.4: 15.27 +/- 0.15 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:46:37.83 +22:25:10.0: 15.11 +/- 0.13 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:37:54.77 +20:14:05.6: 14.77 +/- 0.09 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:52:16.35 +24:48:06.8: 14.93 +/- 0.11 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.10
Forced photometry reference-image weighted average: 15.30 +/- 0.10
Forced photometry reference-image weighted average: 15.02 +/- 0.08
Forced photometry reference-image weighted average: 15.01 +/- 0.08
Forced photometry filter REJECTED candidate at 04:23:43.69 +23:23:32.4: ref_mag=15.31 +/- 0.10 new_mean_mag=15.1740 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:46:42.60 +23:47:52.8: ref_mag=15.30 +/- 0.10 new_mean_mag=15.1126 delta=0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:46:37.83 +22:25:10.0: ref_mag=15.02 +/- 0.08 new_mean_mag=15.0879 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:52:16.35 +24:48:06.8: ref_mag=15.01 +/- 0.08 new_mean_mag=15.1022 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 14.84 +/- 0.06
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:25:14.52 +21:32:48.1: 15.11 +/- 0.12 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:50:59.40 +24:14:00.1: 15.03 +/- 0.13 detection
Forced photometry filter REJECTED candidate at 04:37:54.77 +20:14:05.6: ref_mag=14.84 +/- 0.06 new_mean_mag=14.9510 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:28:28.10 +24:16:21.3: 14.97 +/- 0.11 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.09
Forced photometry reference-image weighted average: 15.17 +/- 0.09
Forced photometry filter REJECTED candidate at 04:50:59.40 +24:14:00.1: ref_mag=15.05 +/- 0.09 new_mean_mag=15.0108 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:25:14.52 +21:32:48.1: ref_mag=15.17 +/- 0.09 new_mean_mag=15.1109 delta=0.05 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:32:53.02 +19:13:37.1: 14.86 +/- 0.10 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:42:54.42 +20:21:12.8: 14.90 +/- 0.10 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.08
Forced photometry filter REJECTED candidate at 04:28:28.10 +24:16:21.3: ref_mag=15.05 +/- 0.08 new_mean_mag=15.1545 delta=-0.10 (need > 0.90)
Forced photometry reference-image weighted average: 14.87 +/- 0.07
Forced photometry reference-image weighted average: 14.97 +/- 0.07
Forced photometry filter REJECTED candidate at 04:32:53.02 +19:13:37.1: ref_mag=14.87 +/- 0.07 new_mean_mag=14.8130 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:42:54.42 +20:21:12.8: ref_mag=14.97 +/- 0.07 new_mean_mag=14.9931 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:05.71 +18:36:27.7: 14.76 +/- 0.09 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:37:00.88 +20:43:44.8: 14.68 +/- 0.09 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:24:04.89 +21:57:38.3: 14.10 +/- 0.04 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:55:55.55 +20:24:50.0: 14.47 +/- 0.07 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:37:52.60 +18:38:22.6: 14.20 +/- 0.05 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:51:16.02 +21:54:19.2: 13.69 +/- 0.03 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:47:41.67 +19:51:06.5: 14.60 +/- 0.08 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:20:19.91 +21:30:59.1: 13.71 +/- 0.03 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:37:00.88 +20:43:44.8: 14.60 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.06
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:21:05.71 +18:36:27.7: 14.55 +/- 0.09 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:18:41.57 +23:57:27.1: 12.37 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 04:37:00.88 +20:43:44.8: ref_mag=14.64 +/- 0.06 new_mean_mag=14.5955 delta=0.05 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:24:04.89 +21:57:38.3: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.06
Forced photometry filter REJECTED candidate at 04:21:05.71 +18:36:27.7: ref_mag=14.65 +/- 0.06 new_mean_mag=14.7927 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 14.04 +/- 0.03
Forced photometry filter REJECTED candidate at 04:24:04.89 +21:57:38.3: ref_mag=14.04 +/- 0.03 new_mean_mag=14.3846 delta=-0.35 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:37:52.60 +18:38:22.6: 14.31 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.04
Forced photometry filter REJECTED candidate at 04:37:52.60 +18:38:22.6: ref_mag=14.25 +/- 0.04 new_mean_mag=14.3580 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:55:55.55 +20:24:50.0: 14.47 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.05
Forced photometry filter REJECTED candidate at 04:55:55.55 +20:24:50.0: ref_mag=14.47 +/- 0.05 new_mean_mag=14.3864 delta=0.08 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:51:16.02 +21:54:19.2: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Forced photometry filter REJECTED candidate at 04:51:16.02 +21:54:19.2: ref_mag=13.70 +/- 0.03 new_mean_mag=13.9780 delta=-0.28 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:47:41.67 +19:51:06.5: 14.38 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.05
Forced photometry filter REJECTED candidate at 04:47:41.67 +19:51:06.5: ref_mag=14.48 +/- 0.05 new_mean_mag=14.6005 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:20:19.91 +21:30:59.1: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.02
Forced photometry filter REJECTED candidate at 04:20:19.91 +21:30:59.1: ref_mag=13.69 +/- 0.02 new_mean_mag=13.8779 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:18:41.57 +23:57:27.1: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter REJECTED candidate at 04:18:41.57 +23:57:27.1: ref_mag=12.33 +/- 0.01 new_mean_mag=12.7346 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:36:58.35 +25:26:36.2: 16.37 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:33:09.76 +25:50:50.9: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:36:58.35 +25:26:36.2: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:54:47.28 +22:58:09.4: 13.89 +/- 0.04 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:54:17.89 +24:00:01.3: 14.07 +/- 0.06 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:33:09.76 +25:50:50.9: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:47:12.04 +18:28:58.5: 13.97 +/- 0.05 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:29:54.33 +26:03:38.2: 14.17 +/- 0.05 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:54:11.07 +23:04:44.6: 14.07 +/- 0.06 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:51:02.05 +24:08:02.4: 14.12 +/- 0.05 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:54:47.28 +22:58:09.4: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.03
Forced photometry filter REJECTED candidate at 04:54:47.28 +22:58:09.4: ref_mag=13.93 +/- 0.03 new_mean_mag=13.8890 delta=0.04 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:54:17.89 +24:00:01.3: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.04
Forced photometry filter REJECTED candidate at 04:54:17.89 +24:00:01.3: ref_mag=13.99 +/- 0.04 new_mean_mag=14.0760 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:23:55.27 +23:01:42.7: 14.24 +/- 0.05 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:47:12.04 +18:28:58.5: 13.91 +/- 0.05 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:47:45.50 +19:20:18.0: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter REJECTED candidate at 04:47:12.04 +18:28:58.5: ref_mag=13.93 +/- 0.04 new_mean_mag=14.0401 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:29:54.33 +26:03:38.2: 14.15 +/- 0.06 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:54:11.07 +23:04:44.6: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.04
Forced photometry filter REJECTED candidate at 04:29:54.33 +26:03:38.2: ref_mag=14.16 +/- 0.04 new_mean_mag=14.2387 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 14.09 +/- 0.04
Forced photometry filter REJECTED candidate at 04:54:11.07 +23:04:44.6: ref_mag=14.09 +/- 0.04 new_mean_mag=14.1881 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:51:02.05 +24:08:02.4: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.04
Forced photometry filter REJECTED candidate at 04:51:02.05 +24:08:02.4: ref_mag=14.08 +/- 0.04 new_mean_mag=14.1829 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:23:55.27 +23:01:42.7: 14.26 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.04
Forced photometry filter REJECTED candidate at 04:23:55.27 +23:01:42.7: ref_mag=14.25 +/- 0.04 new_mean_mag=14.3955 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:47:45.50 +19:20:18.0: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.05
Forced photometry filter REJECTED candidate at 04:47:45.50 +19:20:18.0: ref_mag=14.14 +/- 0.05 new_mean_mag=14.3294 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:47:14.65 +20:33:18.3: 14.19 +/- 0.05 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:52:58.10 +23:28:50.8: 14.46 +/- 0.08 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:44:26.81 +18:49:54.1: 14.33 +/- 0.07 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:42:59.78 +23:02:15.5: 14.19 +/- 0.05 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:49:54.80 +23:17:11.9: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:47:14.65 +20:33:18.3: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.04
Forced photometry filter REJECTED candidate at 04:47:14.65 +20:33:18.3: ref_mag=14.14 +/- 0.04 new_mean_mag=14.3113 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:53:53.99 +21:33:39.3: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:41:53.26 +24:49:15.1: 14.40 +/- 0.07 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:48:48.34 +19:42:37.8: 14.31 +/- 0.07 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:52:58.10 +23:28:50.8: 14.41 +/- 0.08 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:42:59.78 +23:02:15.5: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.06
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:44:26.81 +18:49:54.1: 14.22 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 04:52:58.10 +23:28:50.8: ref_mag=14.44 +/- 0.06 new_mean_mag=14.2938 delta=0.14 (need > 0.90)
Forced photometry reference-image weighted average: 14.15 +/- 0.04
Forced photometry filter REJECTED candidate at 04:42:59.78 +23:02:15.5: ref_mag=14.15 +/- 0.04 new_mean_mag=14.4027 delta=-0.25 (need > 0.90)
Forced photometry reference-image weighted average: 14.27 +/- 0.05
Forced photometry filter REJECTED candidate at 04:44:26.81 +18:49:54.1: ref_mag=14.27 +/- 0.05 new_mean_mag=14.3038 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:49:54.80 +23:17:11.9: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:53:53.99 +21:33:39.3: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:41:53.26 +24:49:15.1: 14.63 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.06
Forced photometry filter REJECTED candidate at 04:41:53.26 +24:49:15.1: ref_mag=14.48 +/- 0.06 new_mean_mag=14.3197 delta=0.16 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:48:48.34 +19:42:37.8: 14.40 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.05
Forced photometry filter REJECTED candidate at 04:48:48.34 +19:42:37.8: ref_mag=14.35 +/- 0.05 new_mean_mag=14.4817 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:27:17.77 +23:02:02.5: 14.39 +/- 0.07 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:29:25.28 +17:51:21.7: 14.35 +/- 0.08 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:25:51.15 +22:09:13.9: 14.75 +/- 0.08 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:27:17.77 +23:02:02.5: 14.33 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.05
Forced photometry filter REJECTED candidate at 04:27:17.77 +23:02:02.5: ref_mag=14.36 +/- 0.05 new_mean_mag=14.4611 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:29:25.28 +17:51:21.7: 14.28 +/- 0.08 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:25:51.15 +22:09:13.9: 14.75 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.06
Forced photometry filter REJECTED candidate at 04:29:25.28 +17:51:21.7: ref_mag=14.32 +/- 0.06 new_mean_mag=14.4437 delta=-0.13 (need > 0.90)
Forced photometry reference-image weighted average: 14.75 +/- 0.06
Forced photometry filter REJECTED candidate at 04:25:51.15 +22:09:13.9: ref_mag=14.75 +/- 0.06 new_mean_mag=14.4913 delta=0.26 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:33:03.61 +17:44:05.3: 14.58 +/- 0.08 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:40:54.48 +20:03:34.3: 14.43 +/- 0.06 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:42:10.20 +22:14:37.0: 14.40 +/- 0.06 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:39:55.57 +23:59:03.0: 14.57 +/- 0.09 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:33:03.61 +17:44:05.3: 14.33 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.05
Forced photometry filter REJECTED candidate at 04:33:03.61 +17:44:05.3: ref_mag=14.45 +/- 0.05 new_mean_mag=14.5113 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:40:54.48 +20:03:34.3: 14.50 +/- 0.08 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:42:10.20 +22:14:37.0: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.05
Forced photometry filter REJECTED candidate at 04:40:54.48 +20:03:34.3: ref_mag=14.46 +/- 0.05 new_mean_mag=14.4996 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.30 +/- 0.04
Forced photometry filter REJECTED candidate at 04:42:10.20 +22:14:37.0: ref_mag=14.30 +/- 0.04 new_mean_mag=14.7389 delta=-0.43 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:29:10.52 +20:42:16.3: 14.93 +/- 0.10 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:39:55.57 +23:59:03.0: 14.44 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.06
Forced photometry filter REJECTED candidate at 04:39:55.57 +23:59:03.0: ref_mag=14.50 +/- 0.06 new_mean_mag=14.5666 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:29:01.51 +19:57:21.7: 14.80 +/- 0.12 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:29:10.52 +20:42:16.3: 14.69 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.06
Forced photometry filter REJECTED candidate at 04:29:10.52 +20:42:16.3: ref_mag=14.79 +/- 0.06 new_mean_mag=14.8568 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:43:54.65 +20:28:55.1: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:33:07.46 +21:24:51.9: 14.62 +/- 0.08 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:20:46.94 +22:24:05.8: 15.61 +/- 0.21 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:29:01.51 +19:57:21.7: 15.01 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.09
Forced photometry filter REJECTED candidate at 04:29:01.51 +19:57:21.7: ref_mag=14.88 +/- 0.09 new_mean_mag=14.7815 delta=0.10 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:33:42.97 +18:45:57.9: 15.25 +/- 0.13 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:43:54.65 +20:28:55.1: 16.20 +/- 0.36 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:33:07.46 +21:24:51.9: 14.68 +/- 0.10 detection
Forced photometry reference-image weighted average: 16.20 +/- 0.36
Forced photometry reference-image weighted average: 14.64 +/- 0.06
Forced photometry filter KEPT candidate at 04:43:54.65 +20:28:55.1: ref_mag=16.20 +/- 0.36 new_mean_mag=14.8507 delta=1.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:33:07.46 +21:24:51.9: ref_mag=14.64 +/- 0.06 new_mean_mag=14.8606 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:20:46.94 +22:24:05.8: 15.81 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.68 +/- 0.16
Forced photometry filter REJECTED candidate at 04:20:46.94 +22:24:05.8: ref_mag=15.68 +/- 0.16 new_mean_mag=15.1563 delta=0.53 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:45.57 +20:58:34.5: 15.27 +/- 0.14 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:33:42.97 +18:45:57.9: 14.90 +/- 0.11 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.08
Forced photometry filter REJECTED candidate at 04:33:42.97 +18:45:57.9: ref_mag=15.04 +/- 0.08 new_mean_mag=15.0036 delta=0.04 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:21:45.57 +20:58:34.5: 15.22 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.10
Forced photometry filter REJECTED candidate at 04:21:45.57 +20:58:34.5: ref_mag=15.24 +/- 0.10 new_mean_mag=14.9719 delta=0.27 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:20:31.01 +19:05:21.7: 15.47 +/- 0.17 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:38:21.80 +17:59:18.7: 15.40 +/- 0.16 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:41:46.65 +21:16:05.6: 14.98 +/- 0.11 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:31:30.48 +20:35:36.9: 15.27 +/- 0.13 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:20:31.01 +19:05:21.7: 15.48 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.47 +/- 0.13
Forced photometry filter REJECTED candidate at 04:20:31.01 +19:05:21.7: ref_mag=15.47 +/- 0.13 new_mean_mag=15.0389 delta=0.44 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:41:46.65 +21:16:05.6: 15.01 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.08
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:38:21.80 +17:59:18.7: 15.70 +/- 0.23 detection
Forced photometry filter REJECTED candidate at 04:41:46.65 +21:16:05.6: ref_mag=14.99 +/- 0.08 new_mean_mag=15.0379 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 15.50 +/- 0.13
Forced photometry filter REJECTED candidate at 04:38:21.80 +17:59:18.7: ref_mag=15.50 +/- 0.13 new_mean_mag=15.0796 delta=0.42 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:36:40.09 +19:27:50.4: 15.18 +/- 0.14 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:31:30.48 +20:35:36.9: 15.25 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.10
Forced photometry filter REJECTED candidate at 04:31:30.48 +20:35:36.9: ref_mag=15.26 +/- 0.10 new_mean_mag=14.9856 delta=0.28 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:36:40.09 +19:27:50.4: 15.22 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.20 +/- 0.10
Forced photometry filter REJECTED candidate at 04:36:40.09 +19:27:50.4: ref_mag=15.20 +/- 0.10 new_mean_mag=14.9916 delta=0.21 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:47.23 +22:29:45.6: 15.61 +/- 0.19 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:18:25.50 +22:55:44.4: 15.72 +/- 0.21 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:43:24.08 +24:54:19.5: 15.37 +/- 0.17 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:52:12.12 +21:32:33.5: 15.54 +/- 0.18 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:21:47.23 +22:29:45.6: 15.67 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.63 +/- 0.15
Forced photometry filter REJECTED candidate at 04:21:47.23 +22:29:45.6: ref_mag=15.63 +/- 0.15 new_mean_mag=15.2080 delta=0.43 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:18:25.50 +22:55:44.4: 14.96 +/- 0.12 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:43:24.08 +24:54:19.5: 15.42 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.10
Forced photometry reference-image weighted average: 15.39 +/- 0.12
Forced photometry filter REJECTED candidate at 04:18:25.50 +22:55:44.4: ref_mag=15.15 +/- 0.10 new_mean_mag=15.1553 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:43:24.08 +24:54:19.5: ref_mag=15.39 +/- 0.12 new_mean_mag=15.2273 delta=0.16 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:19:32.96 +17:54:06.8: 15.40 +/- 0.16 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:52:12.12 +21:32:33.5: 15.52 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.53 +/- 0.13
Forced photometry filter REJECTED candidate at 04:52:12.12 +21:32:33.5: ref_mag=15.53 +/- 0.13 new_mean_mag=15.1115 delta=0.42 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:19:32.96 +17:54:06.8: 15.10 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.11
Forced photometry filter REJECTED candidate at 04:19:32.96 +17:54:06.8: ref_mag=15.23 +/- 0.11 new_mean_mag=15.1402 delta=0.09 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:55:37.92 +22:31:30.1: 15.57 +/- 0.20 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:22.20 +26:06:34.1: 15.61 +/- 0.20 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:55:37.92 +22:31:30.1: 15.24 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.36 +/- 0.12
Forced photometry filter REJECTED candidate at 04:55:37.92 +22:31:30.1: ref_mag=15.36 +/- 0.12 new_mean_mag=15.1012 delta=0.26 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:21:22.20 +26:06:34.1: 15.29 +/- 0.17 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:17:38.07 +22:23:12.4: 15.29 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.42 +/- 0.13
Forced photometry filter REJECTED candidate at 04:21:22.20 +26:06:34.1: ref_mag=15.42 +/- 0.13 new_mean_mag=15.2225 delta=0.20 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:18:19.27 +20:35:24.2: 15.17 +/- 0.13 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:19.63 +20:54:23.4: 15.54 +/- 0.18 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:17:38.07 +22:23:12.4: 15.44 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.35 +/- 0.11
Forced photometry filter REJECTED candidate at 04:17:38.07 +22:23:12.4: ref_mag=15.35 +/- 0.11 new_mean_mag=15.1338 delta=0.21 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:18:19.27 +20:35:24.2: 15.21 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.10
Forced photometry filter REJECTED candidate at 04:18:19.27 +20:35:24.2: ref_mag=15.19 +/- 0.10 new_mean_mag=15.0883 delta=0.10 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:21:19.63 +20:54:23.4: 15.49 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.51 +/- 0.13
Forced photometry filter REJECTED candidate at 04:21:19.63 +20:54:23.4: ref_mag=15.51 +/- 0.13 new_mean_mag=15.2717 delta=0.24 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:42:26.68 +20:47:02.2: 15.20 +/- 0.14 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:54:46.21 +21:09:05.0: 15.68 +/- 0.24 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:42:26.68 +20:47:02.2: 15.16 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.18 +/- 0.10
Forced photometry filter REJECTED candidate at 04:42:26.68 +20:47:02.2: ref_mag=15.18 +/- 0.10 new_mean_mag=15.0815 delta=0.10 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:37:42.20 +20:12:01.7: 15.85 +/- 0.21 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:54:46.21 +21:09:05.0: 15.60 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.64 +/- 0.16
Forced photometry filter REJECTED candidate at 04:54:46.21 +21:09:05.0: ref_mag=15.64 +/- 0.16 new_mean_mag=15.1920 delta=0.45 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:29:34.75 +17:50:17.7: 15.32 +/- 0.18 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:51:37.71 +22:13:23.8: 14.99 +/- 0.11 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:37:42.20 +20:12:01.7: 15.52 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.65 +/- 0.14
Forced photometry filter REJECTED candidate at 04:37:42.20 +20:12:01.7: ref_mag=15.65 +/- 0.14 new_mean_mag=15.2096 delta=0.44 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:29:34.75 +17:50:17.7: 15.10 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.20 +/- 0.12
Forced photometry filter REJECTED candidate at 04:29:34.75 +17:50:17.7: ref_mag=15.20 +/- 0.12 new_mean_mag=15.0709 delta=0.13 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:51:37.71 +22:13:23.8: 14.96 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.08
Forced photometry filter REJECTED candidate at 04:51:37.71 +22:13:23.8: ref_mag=14.98 +/- 0.08 new_mean_mag=15.2218 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:54:47.45 +23:56:58.0: 15.51 +/- 0.22 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:46:48.16 +21:29:31.0: 15.30 +/- 0.19 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:54:47.45 +23:56:58.0: 15.18 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.14
Forced photometry filter REJECTED candidate at 04:54:47.45 +23:56:58.0: ref_mag=15.31 +/- 0.14 new_mean_mag=14.9902 delta=0.32 (need > 0.90)
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-17_23-15-20_20.00sec_-15.00C_LIGHT_0202.fits at 04:46:48.16 +21:29:31.0: 15.35 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.32 +/- 0.14
Forced photometry filter REJECTED candidate at 04:46:48.16 +21:29:31.0: ref_mag=15.32 +/- 0.14 new_mean_mag=15.2416 delta=0.08 (need > 0.90)
Adding exclusion_list_local.txt__out103499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110555.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 100451_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100451_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100454_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100454_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100457_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100457_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100460_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100460_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100463_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100463_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100465_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100465_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100466_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100466_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100468_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100468_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100475_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100475_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100476_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100476_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100480_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100480_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100485_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100485_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100489_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100489_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100492_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100492_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100493_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100493_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 100495_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100495_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100496_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100496_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100500_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100500_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:28:08.36 +20:11:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100503_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100503_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:31:44.30 +25:22:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100504_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100504_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100506_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100506_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 100509_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 100509_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 101194_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 101194_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:28:23.71 +19:10:45.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 102143_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 102143_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:21:45.29 +19:28:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103499_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
Preparing report for the candidate 103499_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
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Considering the candidate 103824_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 103824_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:42:24.72 +22:56:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103909_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 103909_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:55:45.23 +19:58:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104281_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 104281_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:36:07.86 +21:31:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104571_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
Preparing report for the candidate 104571_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
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Considering the candidate 104745_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 104745_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:19:30.06 +21:45:13.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 104833_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 104833_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:25:20.66 +22:10:31.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 104962_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 104962_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:28:14.39 +24:06:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105059_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 105059_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:41:25.51 +18:42:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105085_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 105085_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:55:16.56 +21:52:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105118_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 105118_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:28:27.15 +19:11:38.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 105939_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 105939_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 106113_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 106113_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:19:53.23 +19:30:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106245_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 106245_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:25:38.49 +17:55:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106267_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 106267_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:23:58.65 +24:19:31.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106496_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 106496_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 106804_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 106804_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:53:59.07 +20:19:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106970_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 106970_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 106974_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 106974_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 107045_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 107045_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 107055_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 107055_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:36:57.99 +21:03:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107203_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 107203_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 107280_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 107280_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 107378_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 107378_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 107511_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 107511_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:30:28.44 +23:36:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107812_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 107812_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 107823_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 107823_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 107904_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 107904_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 108121_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108121_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 108125_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
Preparing report for the candidate 108125_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
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Considering the candidate 108249_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108249_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:28:25.73 +19:11:48.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 108291_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
Preparing report for the candidate 108291_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
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Considering the candidate 108317_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108317_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 108319_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108319_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 108342_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108342_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 108391_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108391_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 108428_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108428_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 108464_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108464_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:19:13.89 +23:20:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108571_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108571_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:45:28.70 +20:33:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108701_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108701_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:19:40.58 +21:44:47.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 108717_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108717_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:40:59.20 +18:07:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108771_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 108771_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 109012_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 109012_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 109483_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 109483_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 109727_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 109727_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 109810_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 109810_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:40:37.11 +22:38:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110020_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 110020_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 110112_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 110112_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 110555_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
Preparing report for the candidate 110555_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
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Considering the candidate 110784_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 110784_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 111220_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 111220_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 111535_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 111535_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 111607_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 111607_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 111765_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 111765_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:32:49.12 +22:53:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111786_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 111786_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 111870_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 111870_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 111871_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 111871_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 111894_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 111894_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 111956_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 111956_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 111977_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 111977_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112042_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112042_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112103_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112103_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112154_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112154_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112227_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112227_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112273_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112273_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112349_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112349_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112356_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112356_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 112383_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112383_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112392_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112392_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112440_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112440_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112475_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112475_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112489_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112489_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112679_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112679_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112704_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112704_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112723_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112723_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112730_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112730_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 112734_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 112734_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
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Considering the candidate 60271_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 60271_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:21:25.56 +20:15:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08495_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 08495_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:29:51.55 +26:06:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20082_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 20082_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
**** FOUND 04:34:55.45 +24:28:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73403_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461
The candidate 73403_fd_Tau-03-Q2b1x1_2026-10-12_03-18-04_20.00sec_-0.00C_LIGHT_0461 did not pass the final checks
