This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 03.3175 2461286.8175 11.55 00:07:13.92 -06:25:17.4
94.03987 -66.78053 galactic Cet Second-epoch detections are separated by 0.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.106 Dione -0 0 1 11.8 0 0
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:07:13.92 -06:25:17.4: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:07:13.92 -06:25:17.4: 15.40 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 03.3175* 00 07 13.92 -06 25 17.4 11.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461286.8175,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260903.3175 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.3175 2461286.8175 12.14 23:36:30.72 -08:47:23.6
75.42717 -64.50589 galactic Aqr Second-epoch detections are separated by 0.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.113 Amalthea -0 -0 0 11.9 0 -0
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:36:30.72 -08:47:23.6: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:36:30.72 -08:47:23.6: 15.33 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461286.8175,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260903.3175 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.3175 2461286.8175 11.95 23:58:05.52 -12:34:17.6
79.68264 -70.81698 galactic Cet Second-epoch detections are separated by 1.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.118 Peitho -1 -0 1 12.1 0 -0
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:58:05.52 -12:34:17.6: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:58:05.52 -12:34:17.6: 15.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 03.3175* 23 58 05.52 -12 34 17.6 11.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461286.8175,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260903.3175 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.3175 2461286.8175 12.61 23:34:36.64 -12:01:34.4
69.15774 -66.49302 galactic Aqr Second-epoch detections are separated by 0.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.530 Turandot -0 0 1 12.7 -0 -0
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:34:36.64 -12:01:34.4: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:34:36.64 -12:01:34.4: 15.22 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461286.8175,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260903.3175 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.3175 2461286.8175 13.90 00:19:10.64 -10:00:18.2
97.45619 -71.26336 galactic Cet Second-epoch detections are separated by 2.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1133 Lugduna 0 -0 0 13.8 -0 -0
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:19:10.64 -10:00:18.2: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:19:10.64 -10:00:18.2: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 03.3175* 00 19 10.64 -10 00 18.2 13.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461286.8175,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260903.3175 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 03.3175 2461286.8175 12.41 00:11:24.81 -11:28:43.2
90.00675 -71.74336 galactic Cet Second-epoch detections are separated by 0.4" and 5.4 pix
The object was found in VSX 1" WW Cet
Type: UGZ
# Max. Min./Amp. JD0 Period
10.400 V 15.800 V 0.175780000000 pec(UG)+M2.5V
The object was not found in astcheck.
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:11:24.81 -11:28:43.2: 13.33 +/- 0.05 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:11:24.81 -11:28:43.2: 13.91 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 03.3175* 00 11 24.81 -11 28 43.2 12.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WW Cet,2461286.8175,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WW Cet 20260903.3175 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.93905227 21.07.2026 10:32:04.116 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
First image: 2461242.93905227 21.07.2026 10:32:04.116 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Last image: 2461286.81781953 03.09.2026 07:37:29.607 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 4211
Objects passed selection criteria: 4208
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 3808.5
Average stars matched: 3721.25 (97.7091 %)
Memory usage VmPeak: 230856 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 3 07:02:46 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: 2461242.93905227 21.07.2026 10:32:04.116 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
First image: 2461242.93905227 21.07.2026 10:32:04.116 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Last image: 2461286.81781953 03.09.2026 07:37:29.607 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
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: 10 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): 21875
Objects passed selection criteria: 21815
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 19797.2
Average stars matched: 18984.5 (95.8946 %)
Memory usage VmPeak: 246200 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 3 07:03:43 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
SExtractor catalog cache: saved Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.cat to cache
SExtractor catalog cache: saved Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.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/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461286.81714759
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits exists and is non-empty
wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits exists and is non-empty
wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits exists and is non-empty
wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (1st reference image)
verification OK: wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Image size: 937.6'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:00.437 -10:00:06.37 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits (1st new image)
verification OK: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:11.691 -10:02:57.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.437 -10:00:06.37
Second-epoch image center 00:00:11.691 -10:02:57.79
Angular distance between the image centers 0.0663 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits (2nd new image)
verification OK: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:11.916 -10:02:25.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.437 -10:00:06.37
Second-epoch image center 00:00:11.916 -10:02:25.08
Angular distance between the image centers 0.0609 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 00:00:11.691 -10:02:57.79
Second-epoch second image center 00:00:11.916 -10:02:25.08
Angular distance between the image centers 0.00913 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/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits &> /tmp/tmp.36e0ODq6Nc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits &> /tmp/tmp.QP4k4Qrg81
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits &> /tmp/tmp.zMm51pL3uT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits &> /tmp/tmp.Xqv6UKomqi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
Found non-empty wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
The reference image (wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits) and catalog (wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat) found
'wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 4374 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9535 to 8.0780 deg, Dec -15.2625 to -4.6835 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 351.9535 to 8.0780 deg, Dec -15.2625 to -4.6835 deg
Loaded 4197 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): 3165 out of 3236 total matches.
Matched with Tycho-2 3236 out of 4374 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.569700
a=0.000000 b=1.000000 c=22.569700
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.70
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.70
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 4374 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9535 to 8.0780 deg, Dec -15.2625 to -4.6835 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 351.9535 to 8.0780 deg, Dec -15.2625 to -4.6835 deg
Loaded 4197 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): 3165 out of 3236 total matches.
Matched with Tycho-2 3236 out of 4374 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Forced-photometry filter: calibrated wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits -> calib.txt_param_ref_wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (aperture=7.1)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 4358 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9535 to 8.0779 deg, Dec -15.2626 to -4.6837 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 351.9535 to 8.0779 deg, Dec -15.2626 to -4.6837 deg
Loaded 4197 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): 3202 out of 3251 total matches.
Matched with Tycho-2 3251 out of 4358 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Forced-photometry filter: calibrated wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits -> calib.txt_param_ref_wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.6 pix Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
2.3 pix Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
2.9 pix fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
2.9 pix fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Limiting magnitude estimates:
14.7 mag. Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
14.7 mag. Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
14.2 mag. fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
14.2 mag. fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.36e0ODq6Nc (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/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits' -> 'wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS_IMAGE_NAME=wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS-calibrated image found: wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Checking if the catalog wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat corresponding to the image wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits alredy exist and is non-empty...
Catalog wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat corresponding to the image wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS catalog name: wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=278, bad_region=0, passed=4374
Got 4374 stars (including 4092 good ones) from the SExtractor catalog wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
util/solve_plate_with_UCAC5 got 4374 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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
RA wraps around 0/360 boundary: field RA 351.9535 through 0 to 8.0780, gap 8.0780 to 351.9535
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3993 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3991 matched stars entering correct_measured_positions(), 3991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3991 matched stars entering correct_measured_positions(), 4374 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
RA wraps around 0/360 boundary: field RA 351.9539 through 0 to 8.0777, gap 8.0777 to 351.9539
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3993 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3991 matched stars entering correct_measured_positions(), 4374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 3991 matched stars entering correct_measured_positions(), 4374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 3991 stars left (next iteration limit 4390)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits N_match=3991 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.348 sigma_q2_arcsec=0.331 sigma_q3_arcsec=0.388 sigma_q4_arcsec=0.337 n_q1=1080 n_q2=969 n_q3=999 n_q4=943 worst_quadrant_to_overall_ratio=1.109
The image catalog is written to wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits -region wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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.QP4k4Qrg81 (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/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits' -> 'wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.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/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS_IMAGE_NAME=wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS-calibrated image found: wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Checking if the catalog wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat corresponding to the image wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits alredy exist and is non-empty...
Catalog wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat corresponding to the image wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS catalog name: wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=264, bad_region=0, passed=4358
Got 4358 stars (including 4088 good ones) from the SExtractor catalog wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat
util/solve_plate_with_UCAC5 got 4358 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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
RA wraps around 0/360 boundary: field RA 351.9535 through 0 to 8.0779, gap 8.0779 to 351.9535
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3990 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3988 matched stars entering correct_measured_positions(), 3988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3988 matched stars entering correct_measured_positions(), 4358 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
RA wraps around 0/360 boundary: field RA 351.9539 through 0 to 8.0776, gap 8.0776 to 351.9539
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3990 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3988 matched stars entering correct_measured_positions(), 4358 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 3988 matched stars entering correct_measured_positions(), 4358 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 3988 stars left (next iteration limit 4386)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits N_match=3988 sigma_overall_arcsec=0.291 sigma_q1_arcsec=0.274 sigma_q2_arcsec=0.314 sigma_q3_arcsec=0.312 sigma_q4_arcsec=0.280 n_q1=1022 n_q2=971 n_q3=1079 n_q4=916 worst_quadrant_to_overall_ratio=1.078
The image catalog is written to wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits -region wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.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.zMm51pL3uT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
Checking if the catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
WCS catalog name: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=191, bad_region=0, passed=3306
Got 3306 stars (including 3112 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat
util/solve_plate_with_UCAC5 got 3306 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7372 through 0 to 8.1602, gap 8.1602 to 351.7372
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 371 to 430 (Dec -15.6 to -4.4)
Done reading UCAC5 zone files...
Matched 3026 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3024 matched stars entering correct_measured_positions(), 3024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3024 matched stars entering correct_measured_positions(), 3306 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7369 through 0 to 8.1605, gap 8.1605 to 351.7369
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 371 to 430 (Dec -15.6 to -4.4)
Done reading UCAC5 zone files...
Matched 3027 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3025 matched stars entering correct_measured_positions(), 3306 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 3025 matched stars entering correct_measured_positions(), 3306 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 3025 stars left (next iteration limit 3326)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3025 robust_rms=11.692 arcsec worst_quadrant_rms=14.104 arcsec
SIP_REFIT: SIP order 3 trial: matched=3025 robust_rms=0.377 arcsec worst_quadrant_rms=0.390 arcsec
SIP_REFIT: SIP order 5 trial: matched=3025 robust_rms=0.290 arcsec worst_quadrant_rms=0.334 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3025 robust_rms_before=1.011 arcsec robust_rms_before_corrected=0.284 arcsec robust_rms_after=0.290 arcsec worst_quadrant_rms_before=0.337 worst_quadrant_rms_after=0.334
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.337 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits N_match=3025 sigma_overall_arcsec=0.287 sigma_q1_arcsec=0.329 sigma_q2_arcsec=0.318 sigma_q3_arcsec=0.256 sigma_q4_arcsec=0.258 n_q1=814 n_q2=715 n_q3=830 n_q4=666 worst_quadrant_to_overall_ratio=1.145
The image catalog is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits -region wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.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.Xqv6UKomqi (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Checking if the catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
WCS catalog name: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=190, bad_region=0, passed=3296
Got 3296 stars (including 3102 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat
util/solve_plate_with_UCAC5 got 3296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7371 through 0 to 8.1601, gap 8.1601 to 351.7371
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 372 to 429 (Dec -15.6 to -4.4)
Done reading UCAC5 zone files...
Matched 3017 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3015 matched stars entering correct_measured_positions(), 3015 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3015 matched stars entering correct_measured_positions(), 3296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7367 through 0 to 8.1605, gap 8.1605 to 351.7367
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 372 to 429 (Dec -15.6 to -4.4)
Done reading UCAC5 zone files...
Matched 3018 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3016 matched stars entering correct_measured_positions(), 3296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 3016 matched stars entering correct_measured_positions(), 3296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 3016 stars left (next iteration limit 3316)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3016 robust_rms=11.697 arcsec worst_quadrant_rms=13.805 arcsec
SIP_REFIT: SIP order 3 trial: matched=3016 robust_rms=0.381 arcsec worst_quadrant_rms=0.394 arcsec
SIP_REFIT: SIP order 5 trial: matched=3016 robust_rms=0.300 arcsec worst_quadrant_rms=0.338 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3016 robust_rms_before=1.015 arcsec robust_rms_before_corrected=0.282 arcsec robust_rms_after=0.300 arcsec worst_quadrant_rms_before=0.330 worst_quadrant_rms_after=0.338
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.330 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits N_match=3016 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.320 sigma_q3_arcsec=0.262 sigma_q4_arcsec=0.259 n_q1=808 n_q2=708 n_q3=834 n_q4=666 worst_quadrant_to_overall_ratio=1.126
The image catalog is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits -region wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.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_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits to local_wcs_cache/
'wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits' -> 'local_wcs_cache/wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits'
Saving the final (post-refit) wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits to local_wcs_cache/
'wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits' -> 'local_wcs_cache/wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits'
Saving the final (post-refit) wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits to local_wcs_cache/
'wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits' -> 'local_wcs_cache/wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits'
Saving the final (post-refit) wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits to local_wcs_cache/
'wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits' -> 'local_wcs_cache/wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits sigma_overall=0.350 worst_q_ratio=1.109
ref2=Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits sigma_overall=0.291 worst_q_ratio=1.078
new1=fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits sigma_overall=0.287 worst_q_ratio=1.145
new2=fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits sigma_overall=0.286 worst_q_ratio=1.126
reference average sigma_overall=0.3205 worst_q_ratio=1.0935
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021_astrometric_residuals.png (3991 matched stars from wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490_astrometric_residuals.png (3988 matched stars from wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285_astrometric_residuals.png (3025 matched stars from wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286_astrometric_residuals.png (3016 matched stars from wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits'
Saving fully-calibrated image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits'
Preparing the HTML report for the field Cet-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:07:13.92 -06:25:17.4: 15.38 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:07:13.92 -06:25:17.4: 15.40 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20309.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20309_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
Preparing report for the candidate 20309_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00255_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 00255_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
**** FOUND 00:02:07.32 -14:40:30.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03145_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 03145_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
**** FOUND 00:13:45.95 -07:48:34.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Cet-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:07:13.92 -06:25:17.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
SExtractor catalog cache: saved Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.cat to cache
SExtractor catalog cache: saved Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Creating symlink local_wcs_cache/wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits exists and is non-empty
wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits exists and is non-empty
wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits exists and is non-empty
wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (1st reference image)
verification OK: wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Image size: 937.6'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:00.437 -10:00:06.37 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits (1st new image)
verification OK: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:11.691 -10:02:57.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.437 -10:00:06.37
Second-epoch image center 00:00:11.691 -10:02:57.79
Angular distance between the image centers 0.0663 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits (2nd new image)
verification OK: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:11.916 -10:02:25.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.437 -10:00:06.37
Second-epoch image center 00:00:11.916 -10:02:25.08
Angular distance between the image centers 0.0609 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 00:00:11.691 -10:02:57.79
Second-epoch second image center 00:00:11.916 -10:02:25.08
Angular distance between the image centers 0.00913 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/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits &> /tmp/tmp.BgJHO1Dl47
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits &> /tmp/tmp.o44Eyai7GJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits &> /tmp/tmp.2fYZeQfbWd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits &> /tmp/tmp.eboziEjmqs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
Found non-empty wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
The reference image (wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits) and catalog (wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat) found
'wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 22737 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9459 to 8.0985 deg, Dec -15.2699 to -4.6646 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 351.9459 to 8.0985 deg, Dec -15.2699 to -4.6646 deg
Loaded 4214 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): 3418 out of 3629 total matches.
Matched with Tycho-2 3629 out of 22737 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.388800
a=0.000000 b=1.000000 c=22.388800
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.83
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.83
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 22737 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9459 to 8.0985 deg, Dec -15.2699 to -4.6646 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 351.9459 to 8.0985 deg, Dec -15.2699 to -4.6646 deg
Loaded 4214 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): 3418 out of 3629 total matches.
Matched with Tycho-2 3629 out of 22737 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Forced-photometry filter: calibrated wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits -> calib.txt_param_ref_wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (aperture=5.3)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 23415 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9462 to 8.0901 deg, Dec -15.2699 to -4.6646 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 351.9462 to 8.0901 deg, Dec -15.2699 to -4.6646 deg
Loaded 4212 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): 3459 out of 3633 total matches.
Matched with Tycho-2 3633 out of 23415 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Forced-photometry filter: calibrated wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits -> calib.txt_param_ref_wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 28 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
2.2 pix Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
2.7 pix fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
2.6 pix fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Limiting magnitude estimates:
14.8 mag. Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
14.9 mag. Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
14.4 mag. fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
14.4 mag. fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BgJHO1Dl47 (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/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits' -> 'wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS_IMAGE_NAME=wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS-calibrated image found: wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Checking if the catalog wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat corresponding to the image wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits alredy exist and is non-empty...
Catalog wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat corresponding to the image wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS catalog name: wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=913, bad_region=0, passed=22729
Got 22729 stars (including 21779 good ones) from the SExtractor catalog wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
util/solve_plate_with_UCAC5 got 22729 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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
RA wraps around 0/360 boundary: field RA 351.9459 through 0 to 8.0985, gap 8.0985 to 351.9459
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 22729 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
RA wraps around 0/360 boundary: field RA 351.9463 through 0 to 8.0982, gap 8.0982 to 351.9463
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 22729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 22729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4864 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits N_match=4864 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.355 sigma_q2_arcsec=0.325 sigma_q3_arcsec=0.415 sigma_q4_arcsec=0.337 n_q1=1269 n_q2=1240 n_q3=1176 n_q4=1179 worst_quadrant_to_overall_ratio=1.175
The image catalog is written to wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits -region wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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.o44Eyai7GJ (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/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits' -> 'wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.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/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS_IMAGE_NAME=wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS-calibrated image found: wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Checking if the catalog wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat corresponding to the image wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits alredy exist and is non-empty...
Catalog wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat corresponding to the image wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS catalog name: wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=831, bad_region=0, passed=23408
Got 23408 stars (including 22542 good ones) from the SExtractor catalog wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat
util/solve_plate_with_UCAC5 got 23408 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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
RA wraps around 0/360 boundary: field RA 351.9462 through 0 to 8.0901, gap 8.0901 to 351.9462
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 4860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 23408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9465 through 0 to 8.0899, gap 8.0899 to 351.9465
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 23408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 23408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4860 stars left (next iteration limit 5346)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.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_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits N_match=4860 sigma_overall_arcsec=0.295 sigma_q1_arcsec=0.270 sigma_q2_arcsec=0.305 sigma_q3_arcsec=0.327 sigma_q4_arcsec=0.297 n_q1=1259 n_q2=1185 n_q3=1245 n_q4=1171 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits -region wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.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.2fYZeQfbWd (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
Checking if the catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
WCS catalog name: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=530, bad_region=3, passed=16839
Got 16839 stars (including 16287 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat
util/solve_plate_with_UCAC5 got 16839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7029 through 0 to 8.2165, gap 8.2165 to 351.7029
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 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 4866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 16839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7024 through 0 to 8.2168, gap 8.2168 to 351.7024
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 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 16839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 16839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4864 stars left (next iteration limit 5351)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.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=4864 robust_rms=11.106 arcsec worst_quadrant_rms=12.755 arcsec
SIP_REFIT: SIP order 3 trial: matched=4864 robust_rms=0.425 arcsec worst_quadrant_rms=0.443 arcsec
SIP_REFIT: SIP order 5 trial: matched=4864 robust_rms=0.333 arcsec worst_quadrant_rms=0.404 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4864 robust_rms_before=1.040 arcsec robust_rms_before_corrected=0.330 arcsec robust_rms_after=0.333 arcsec worst_quadrant_rms_before=0.408 worst_quadrant_rms_after=0.404
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.408 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits N_match=4864 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.290 sigma_q4_arcsec=0.287 n_q1=1205 n_q2=1106 n_q3=1386 n_q4=1167 worst_quadrant_to_overall_ratio=1.183
The image catalog is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits -region wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.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.eboziEjmqs (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Checking if the catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
WCS catalog name: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=495, bad_region=4, passed=16863
Got 16863 stars (including 16339 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat
util/solve_plate_with_UCAC5 got 16863 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7030 through 0 to 8.2165, gap 8.2165 to 351.7030
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 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 16863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.7024 through 0 to 8.2169, gap 8.2169 to 351.7024
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 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 16863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 16863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4864 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.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=4864 robust_rms=11.001 arcsec worst_quadrant_rms=12.729 arcsec
SIP_REFIT: SIP order 3 trial: matched=4864 robust_rms=0.425 arcsec worst_quadrant_rms=0.441 arcsec
SIP_REFIT: SIP order 5 trial: matched=4864 robust_rms=0.342 arcsec worst_quadrant_rms=0.399 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4864 robust_rms_before=1.040 arcsec robust_rms_before_corrected=0.333 arcsec robust_rms_after=0.342 arcsec worst_quadrant_rms_before=0.401 worst_quadrant_rms_after=0.399
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.401 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits N_match=4864 sigma_overall_arcsec=0.330 sigma_q1_arcsec=0.394 sigma_q2_arcsec=0.357 sigma_q3_arcsec=0.314 sigma_q4_arcsec=0.289 n_q1=1213 n_q2=1104 n_q3=1381 n_q4=1166 worst_quadrant_to_overall_ratio=1.192
The image catalog is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits -region wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.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_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-36-31_20.00sec_-0.00C_LIGHTs_0285.fits
Saving fully-calibrated image wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Cet-05-Q1b1x1_070013_TTUQ1b1x1_921504_tvQyYjau/wcs_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286.fits
Preparing the HTML report for the field Cet-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:58:05.52 -12:34:17.6: 15.49 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:59:45.78 -05:52:35.1: 12.56 +/- 0.03 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:36:30.72 -08:47:23.6: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:52:48.93 -06:31:08.6: 13.27 +/- 0.05 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:34:36.64 -12:01:34.4: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:51:01.61 -05:38:19.7: 12.78 +/- 0.03 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:48:06.66 -07:36:47.6: 12.84 +/- 0.04 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:44:45.09 -06:55:28.0: 13.39 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:35:11.84 -09:41:22.4: 13.19 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:41:57.22 -07:37:14.8: 12.72 +/- 0.03 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:36:30.72 -08:47:23.6: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:58:05.52 -12:34:17.6: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:51:01.61 -05:38:19.7: 12.97 +/- 0.04 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:34:36.64 -12:01:34.4: 15.22 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:59:45.78 -05:52:35.1: 12.52 +/- 0.03 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:48:06.66 -07:36:47.6: 13.02 +/- 0.04 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:52:48.93 -06:31:08.6: 13.23 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.03
Forced photometry reference-image weighted average: 12.54 +/- 0.02
Forced photometry reference-image weighted average: 12.92 +/- 0.03
Forced photometry filter REJECTED candidate at 23:51:01.61 -05:38:19.7: ref_mag=12.86 +/- 0.03 new_mean_mag=13.3449 delta=-0.48 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:59:45.78 -05:52:35.1: ref_mag=12.54 +/- 0.02 new_mean_mag=12.5613 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Forced photometry filter REJECTED candidate at 23:48:06.66 -07:36:47.6: ref_mag=12.92 +/- 0.03 new_mean_mag=13.1958 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:52:48.93 -06:31:08.6: ref_mag=13.24 +/- 0.03 new_mean_mag=13.3051 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:41:57.22 -07:37:14.8: 12.87 +/- 0.04 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:35:11.84 -09:41:22.4: 13.24 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:44:45.09 -06:55:28.0: 13.41 +/- 0.06 detection
Forced photometry filter REJECTED candidate at 23:41:57.22 -07:37:14.8: ref_mag=12.79 +/- 0.02 new_mean_mag=13.3984 delta=-0.61 (need > 0.90)
Forced photometry reference-image weighted average: 13.22 +/- 0.05
Forced photometry reference-image weighted average: 13.40 +/- 0.04
Forced photometry filter REJECTED candidate at 23:35:11.84 -09:41:22.4: ref_mag=13.22 +/- 0.05 new_mean_mag=13.2024 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:44:45.09 -06:55:28.0: ref_mag=13.40 +/- 0.04 new_mean_mag=13.5422 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:41:25.03 -06:14:31.2: 14.53 +/- 0.18 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:35:14.17 -04:49:07.3: 14.48 +/- 0.20 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:19:10.64 -10:00:18.2: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:00:47.29 -09:01:10.9: 13.69 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:36:15.70 -06:51:52.2: 14.55 +/- 0.19 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:43:59.43 -08:18:30.1: 14.56 +/- 0.18 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:52:43.38 -06:40:27.4: 14.35 +/- 0.14 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:35:14.17 -04:49:07.3: 14.36 +/- 0.17 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:41:25.03 -06:14:31.2: 14.49 +/- 0.17 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:19:10.64 -10:00:18.2: 15.47 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.42 +/- 0.13
Forced photometry reference-image weighted average: 14.51 +/- 0.12
Forced photometry filter REJECTED candidate at 23:35:14.17 -04:49:07.3: ref_mag=14.42 +/- 0.13 new_mean_mag=14.2760 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:41:25.03 -06:14:31.2: ref_mag=14.51 +/- 0.12 new_mean_mag=14.1505 delta=0.36 (need > 0.90)
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:00:47.29 -09:01:10.9: 13.83 +/- 0.08 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:43:59.43 -08:18:30.1: 14.36 +/- 0.14 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:52:43.38 -06:40:27.4: 14.20 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.05
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:36:15.70 -06:51:52.2: 14.67 +/- 0.19 detection
Forced photometry filter REJECTED candidate at 00:00:47.29 -09:01:10.9: ref_mag=13.75 +/- 0.05 new_mean_mag=13.9403 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 14.44 +/- 0.11
Forced photometry reference-image weighted average: 14.26 +/- 0.09
Forced photometry filter REJECTED candidate at 23:43:59.43 -08:18:30.1: ref_mag=14.44 +/- 0.11 new_mean_mag=14.2704 delta=0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:52:43.38 -06:40:27.4: ref_mag=14.26 +/- 0.09 new_mean_mag=14.2282 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.61 +/- 0.13
Forced photometry filter REJECTED candidate at 23:36:15.70 -06:51:52.2: ref_mag=14.61 +/- 0.13 new_mean_mag=14.2878 delta=0.32 (need > 0.90)
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:31:52.58 -05:46:38.4: 14.26 +/- 0.15 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:31:36.10 -10:20:02.7: 13.94 +/- 0.11 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:41:29.79 -06:53:05.8: 14.65 +/- 0.19 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:56:18.93 -09:31:10.8: 13.84 +/- 0.09 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:31:52.58 -05:46:38.4: 14.45 +/- 0.18 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:31:36.10 -10:20:02.7: 13.97 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.12
Forced photometry filter REJECTED candidate at 23:31:52.58 -05:46:38.4: ref_mag=14.34 +/- 0.12 new_mean_mag=14.2798 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.96 +/- 0.08
Forced photometry filter REJECTED candidate at 23:31:36.10 -10:20:02.7: ref_mag=13.96 +/- 0.08 new_mean_mag=14.1325 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:41:29.79 -06:53:05.8: 14.69 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.13
Forced photometry filter REJECTED candidate at 23:41:29.79 -06:53:05.8: ref_mag=14.67 +/- 0.13 new_mean_mag=14.2729 delta=0.40 (need > 0.90)
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:56:18.93 -09:31:10.8: 13.78 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.06
Forced photometry filter REJECTED candidate at 23:56:18.93 -09:31:10.8: ref_mag=13.81 +/- 0.06 new_mean_mag=13.8816 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:11:24.81 -11:28:43.2: 13.33 +/- 0.05 detection
Forced photometry on wcs_Cet-05-Q1b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:11:24.81 -11:28:43.2: 13.91 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.04
Forced photometry filter KEPT candidate at 00:11:24.81 -11:28:43.2: ref_mag=13.47 +/- 0.04 new_mean_mag=12.4140 delta=1.05 (need > 0.90)
Adding exclusion_list_local.txt__out08581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32881.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32381_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32381_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
**** FOUND 00:19:24.42 -08:51:12.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32432_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32432_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
**** FOUND 00:07:13.92 -06:25:17.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32475_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
Preparing report for the candidate 32475_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32494_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
Preparing report for the candidate 32494_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32535_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32535_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32545_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32545_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
**** FOUND 00:05:10.85 -05:41:48.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32559_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
Preparing report for the candidate 32559_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32673_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32673_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32678_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32678_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32702_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32702_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32710_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32710_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32737_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32737_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32744_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32744_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32844_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32844_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32881_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
Preparing report for the candidate 32881_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32884_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32884_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32900_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32900_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32901_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32901_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32917_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32917_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32919_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32919_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32922_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32922_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32925_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32925_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32929_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32929_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32931_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32931_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32933_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 32933_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01200_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 01200_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
**** FOUND 00:02:07.33 -14:40:30.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21120_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286
The candidate 21120_fd_Cet-05-Q1b1x1_2026-09-03_02-37-29_20.00sec_-0.00C_LIGHTs_0286 did not pass the final checks
