This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1
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 06 12.3274 2461203.8274 11.59 15:22:35.42 -08:58:21.7
353.66793 38.58082 galactic Lib Second-epoch detections are separated by 0.2" and 3.4 pix
The object was found in VSX18" Gaia DR3 6320860733384541440
Type: E
# Max. Min./Amp. JD0 Period
15.970 G 16.790 G 0.438476000000 K
The object was found in astcheck.92 Undina -0 -0 0 11.7 -0 0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:22:35.42 -08:58:21.7: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:22:35.42 -08:58:21.7: 15.61 +/- 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
Gaia DR3 6320860733384541440,2461203.8274,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6320860733384541440 20260612.3274 11.59CV 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 06 12.3274 2461203.8274 11.94 15:41:17.78 -13:31:04.6
353.74657 32.12478 galactic Lib Second-epoch detections are separated by 0.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.346 Hermentaria -0 -0 0 11.8 -0 -0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:41:17.78 -13:31:04.6: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:41:17.78 -13:31:04.6: 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!
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,2461203.8274,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260612.3274 11.94CV 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 06 12.3274 2461203.8274 12.84 15:23:53.60 -09:33:14.4
353.44546 37.93991 galactic Lib Second-epoch detections are separated by 0.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.776 Berbericia -0 -1 1 12.8 -0 0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:23:53.60 -09:33:14.4: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:23:53.60 -09:33:14.4: 15.84 +/- 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,2461203.8274,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260612.3274 12.84CV 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 06 12.3274 2461203.8274 13.09 15:43:25.56 -08:38:15.4
358.43198 35.10406 galactic Lib Second-epoch detections are separated by 0.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.559 Nanon 0 -0 0 13.2 0 -0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:43:25.56 -08:38:15.4: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:43:25.56 -08:38:15.4: 15.71 +/- 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,2461203.8274,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260612.3274 13.09CV 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 06 12.3274 2461203.8274 13.32 15:32:48.53 -13:20:54.0
352.13512 33.69263 galactic Lib Second-epoch detections are separated by 0.1" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.563 Suleika 0 -0 0 13.5 -0 -0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:32:48.53 -13:20:54.0: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:32:48.53 -13:20:54.0: 15.65 +/- 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,2461203.8274,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260612.3274 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 12.3274 2461203.8274 12.57 15:11:45.26 -07:46:50.2
352.20676 41.29176 galactic Lib Second-epoch detections are separated by 0.5" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.269 Justitia 0 0 0 12.6 -0 0
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:11:45.26 -07:46:50.2: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:11:45.26 -07:46:50.2: 15.86 +/- 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,2461203.8274,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260612.3274 12.57CV 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: 2461153.89842042 23.04.2026 09:33:33.524 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
First image: 2461153.89842042 23.04.2026 09:33:33.524 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Last image: 2461203.82758851 12.06.2026 07:51:33.647 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 6100
Objects passed selection criteria: 6096
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 5796.5
Average stars matched: 5641.75 (97.3303 %)
Memory usage VmPeak: 112628 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jun 12 07:25:08 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: 2461153.89842042 23.04.2026 09:33:33.524 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
First image: 2461153.89842042 23.04.2026 09:33:33.524 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Last image: 2461203.82758851 12.06.2026 07:51:33.647 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 73
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 26 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 42640
Objects passed selection criteria: 42552
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 41100.5
Average stars matched: 39876 (97.0207 %)
Memory usage VmPeak: 145980 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jun 12 07:28:05 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
SExtractor catalog cache: saved Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat to cache
SExtractor catalog cache: saved Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.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/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.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: 2461203.82716373
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits exists and is non-empty
Saving wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits to local_wcs_cache/
'wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits' -> 'local_wcs_cache/wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits'
wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits exists and is non-empty
Saving wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits to local_wcs_cache/
'wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits' -> 'local_wcs_cache/wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits'
wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits exists and is non-empty
Saving wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits to local_wcs_cache/
'wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits' -> 'local_wcs_cache/wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits'
wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits exists and is non-empty
Saving wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits to local_wcs_cache/
'wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits' -> 'local_wcs_cache/wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits (1st reference image)
verification OK: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:25:43.642 -10:00:07.17 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits (1st new image)
verification OK: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:26:02.676 -10:00:29.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:43.642 -10:00:07.17
Second-epoch image center 15:26:02.676 -10:00:29.98
Angular distance between the image centers 0.0784 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits (2nd new image)
verification OK: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:26:03.961 -10:00:25.03 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:43.642 -10:00:07.17
Second-epoch image center 15:26:03.961 -10:00:25.03
Angular distance between the image centers 0.0835 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 15:26:02.676 -10:00:29.98
Second-epoch second image center 15:26:03.961 -10:00:25.03
Angular distance between the image centers 0.00545 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits &> /tmp/tmp.uGfLKDPHPu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits &> /tmp/tmp.3MOT3YuoU3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits &> /tmp/tmp.nnUlaPOF3y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits &> /tmp/tmp.PHuKly92UG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.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_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.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_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat
Found non-empty wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat
The reference image (wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits) and catalog (wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat) found
'wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat' -> 'wcsmag.cat'
Read 8132 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 222.9892 to 239.6626 deg, Dec -15.6642 to -4.1937 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 222.9892 to 239.6626 deg, Dec -15.6642 to -4.1937 deg
Loaded 6002 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): 4551 out of 4710 total matches.
Matched with Tycho-2 4710 out of 8132 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.736000
a=0.000000 b=1.000000 c=22.736000
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8132 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 222.9892 to 239.6626 deg, Dec -15.6642 to -4.1937 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 222.9892 to 239.6626 deg, Dec -15.6642 to -4.1937 deg
Loaded 6002 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): 4551 out of 4710 total matches.
Matched with Tycho-2 4710 out of 8132 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits:
Forced-photometry filter: calibrated wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits -> calib.txt_param_ref_wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits (aperture=5.9)
Read 8122 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.3808 to 239.4992 deg, Dec -15.2688 to -4.7095 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 223.3808 to 239.4992 deg, Dec -15.2688 to -4.7095 deg
Loaded 5366 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): 4509 out of 4666 total matches.
Matched with Tycho-2 4666 out of 8122 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits:
Forced-photometry filter: calibrated wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits -> calib.txt_param_ref_wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
2.2 pix Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
2.3 pix fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
2.4 pix fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
2.2 pix wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
2.2 pix wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Limiting magnitude estimates:
15.1 mag. Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
15.0 mag. Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
14.7 mag. fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
14.7 mag. fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.uGfLKDPHPu (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/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits' -> 'wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS_IMAGE_NAME=wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS-calibrated image found: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Checking if the catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat corresponding to the image wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits alredy exist and is non-empty...
Catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat corresponding to the image wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS catalog name: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=500, passed=8132
Got 8132 stars (including 7623 good ones) from the SExtractor catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 8132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 7988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 7988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 7988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits N_match=967 sigma_overall_arcsec=0.261 sigma_q1_arcsec=0.252 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.225 sigma_q4_arcsec=0.221 n_q1=252 n_q2=185 n_q3=262 n_q4=268 worst_quadrant_to_overall_ratio=1.342
The image catalog is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits -region wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3MOT3YuoU3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits' -> 'wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS_IMAGE_NAME=wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS-calibrated image found: wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Checking if the catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat corresponding to the image wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits alredy exist and is non-empty...
Catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat corresponding to the image wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS catalog name: wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=502, passed=8122
Got 8122 stars (including 7614 good ones) from the SExtractor catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat
util/solve_plate_with_UCAC5 got 8122 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 8023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 8023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 8023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits N_match=968 sigma_overall_arcsec=0.444 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.609 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.538 n_q1=226 n_q2=215 n_q3=242 n_q4=285 worst_quadrant_to_overall_ratio=1.371
The image catalog is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits -region wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nnUlaPOF3y (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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
WCS_IMAGE_NAME=wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
WCS-calibrated image found: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
Checking if the catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
WCS catalog name: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=377, passed=6685
Got 6685 stars (including 6305 good ones) from the SExtractor catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat
util/solve_plate_with_UCAC5 got 6685 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6611 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6610 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6610 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits N_match=969 sigma_overall_arcsec=0.507 sigma_q1_arcsec=0.426 sigma_q2_arcsec=0.619 sigma_q3_arcsec=0.451 sigma_q4_arcsec=0.560 n_q1=234 n_q2=218 n_q3=229 n_q4=288 worst_quadrant_to_overall_ratio=1.221
The image catalog is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits -region wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PHuKly92UG (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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
WCS-calibrated image found: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
Checking if the catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
WCS catalog name: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=376, passed=6723
Got 6723 stars (including 6343 good ones) from the SExtractor catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 6723 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6635 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6633 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 6633 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits N_match=969 sigma_overall_arcsec=0.462 sigma_q1_arcsec=0.404 sigma_q2_arcsec=0.515 sigma_q3_arcsec=0.378 sigma_q4_arcsec=0.510 n_q1=233 n_q2=214 n_q3=235 n_q4=287 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits -region wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits sigma_overall=0.261 worst_q_ratio=1.342
ref2=Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits sigma_overall=0.444 worst_q_ratio=1.371
new1=fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits sigma_overall=0.507 worst_q_ratio=1.221
new2=fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits sigma_overall=0.462 worst_q_ratio=1.116
reference average sigma_overall=0.3525 worst_q_ratio=1.3565
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258_astrometric_residuals.png (967 matched stars from wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275_astrometric_residuals.png (968 matched stars from wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136_astrometric_residuals.png (969 matched stars from wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137_astrometric_residuals.png (969 matched stars from wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits'
Saving fully-calibrated image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits'
Preparing the HTML report for the field Lib-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:22:35.42 -08:58:21.7: 15.69 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:41:17.78 -13:31:04.6: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:22:35.42 -08:58:21.7: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:41:17.78 -13:31:04.6: 15.45 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20586.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20576_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
Preparing report for the candidate 20576_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20586_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
Preparing report for the candidate 20586_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Lib-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
15:22:35.42 -08:58:21.7
15:41:17.78 -13:31:04.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
SExtractor catalog cache: saved Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.cat to cache
SExtractor catalog cache: saved Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Creating symlink local_wcs_cache/wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits exists and is non-empty
wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits exists and is non-empty
wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits exists and is non-empty
wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits (1st reference image)
verification OK: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:25:43.642 -10:00:07.17 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits (1st new image)
verification OK: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:26:02.676 -10:00:29.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:43.642 -10:00:07.17
Second-epoch image center 15:26:02.676 -10:00:29.98
Angular distance between the image centers 0.0784 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits (2nd new image)
verification OK: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:26:03.961 -10:00:25.03 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:43.642 -10:00:07.17
Second-epoch image center 15:26:03.961 -10:00:25.03
Angular distance between the image centers 0.0835 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 15:26:02.676 -10:00:29.98
Second-epoch second image center 15:26:03.961 -10:00:25.03
Angular distance between the image centers 0.00545 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits &> /tmp/tmp.ABzgYbL0oz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits &> /tmp/tmp.PHwDf1poWm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits &> /tmp/tmp.EfNc6BjTUn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits &> /tmp/tmp.dICcLwpd4w
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.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_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.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_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat
Found non-empty wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits and wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat
The reference image (wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits) and catalog (wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat) found
'wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat' -> 'wcsmag.cat'
Read 56059 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 222.9892 to 239.6626 deg, Dec -15.6809 to -4.1523 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 222.9892 to 239.6626 deg, Dec -15.6809 to -4.1523 deg
Loaded 6037 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): 4376 out of 4830 total matches.
Matched with Tycho-2 4830 out of 56059 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.606950
a=0.000000 b=1.000000 c=22.606950
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 56059 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 222.9892 to 239.6626 deg, Dec -15.6809 to -4.1523 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 222.9892 to 239.6626 deg, Dec -15.6809 to -4.1523 deg
Loaded 6037 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): 4376 out of 4830 total matches.
Matched with Tycho-2 4830 out of 56059 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits:
Forced-photometry filter: calibrated wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits -> calib.txt_param_ref_wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits (aperture=4.5)
Read 50094 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.3438 to 239.5045 deg, Dec -15.2716 to -4.7095 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 223.3438 to 239.5045 deg, Dec -15.2716 to -4.7095 deg
Loaded 5381 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): 4369 out of 4768 total matches.
Matched with Tycho-2 4768 out of 50094 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits:
Forced-photometry filter: calibrated wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits -> calib.txt_param_ref_wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
2.1 pix Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
2.1 pix fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
2.2 pix fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
2.0 pix wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
2.1 pix wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Limiting magnitude estimates:
15.2 mag. Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
15.2 mag. Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
15.0 mag. fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
14.9 mag. fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.4 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ABzgYbL0oz (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/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits' -> 'wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS_IMAGE_NAME=wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS-calibrated image found: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
Checking if the catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat corresponding to the image wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits alredy exist and is non-empty...
Catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat corresponding to the image wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits
WCS catalog name: wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=2373, passed=56051
Got 56051 stars (including 53576 good ones) from the SExtractor catalog wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 56051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 55262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 55261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 55261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits N_match=971 sigma_overall_arcsec=0.261 sigma_q1_arcsec=0.241 sigma_q2_arcsec=0.349 sigma_q3_arcsec=0.216 sigma_q4_arcsec=0.252 n_q1=258 n_q2=191 n_q3=251 n_q4=271 worst_quadrant_to_overall_ratio=1.341
The image catalog is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits -region wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PHwDf1poWm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits' -> 'wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS_IMAGE_NAME=wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS-calibrated image found: wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
Checking if the catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat corresponding to the image wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits alredy exist and is non-empty...
Catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat corresponding to the image wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits
WCS catalog name: wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2552, passed=50088
Got 50088 stars (including 47468 good ones) from the SExtractor catalog wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat
util/solve_plate_with_UCAC5 got 50088 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 49374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 49371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 49371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits N_match=972 sigma_overall_arcsec=0.453 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.593 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.577 n_q1=252 n_q2=202 n_q3=251 n_q4=267 worst_quadrant_to_overall_ratio=1.309
The image catalog is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits -region wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EfNc6BjTUn (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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
WCS_IMAGE_NAME=wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
WCS-calibrated image found: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
Checking if the catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
WCS catalog name: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1810, passed=44625
Got 44625 stars (including 42764 good ones) from the SExtractor catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat
util/solve_plate_with_UCAC5 got 44625 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 44148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 44145 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 44145 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits N_match=972 sigma_overall_arcsec=0.502 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.591 sigma_q3_arcsec=0.445 sigma_q4_arcsec=0.546 n_q1=252 n_q2=218 n_q3=227 n_q4=275 worst_quadrant_to_overall_ratio=1.178
The image catalog is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits -region wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dICcLwpd4w (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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
WCS-calibrated image found: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
Checking if the catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat corresponding to the image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
WCS catalog name: wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1793, passed=43936
Got 43936 stars (including 42085 good ones) from the SExtractor catalog wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 43936 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 43346 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 43345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 43345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits N_match=970 sigma_overall_arcsec=0.458 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.472 sigma_q3_arcsec=0.414 sigma_q4_arcsec=0.505 n_q1=253 n_q2=216 n_q3=230 n_q4=271 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits -region wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-50-56_20.00sec_5.00C_LIGHT_0136.fits
Saving fully-calibrated image wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.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_2026-06-12_CI_Lib-02-Q2b1x1_030446_TTUQ2b1x1_2654531_4R4sVuD1/wcs_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137.fits
Preparing the HTML report for the field Lib-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:48:02.57 -08:43:07.3: 13.03 +/- 0.03 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:41:25.81 -12:45:03.1: 13.97 +/- 0.07 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:47:34.83 -12:05:12.3: 12.38 +/- 0.02 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:44:04.53 -09:36:48.2: 13.20 +/- 0.03 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:14:14.08 -11:48:59.1: 13.07 +/- 0.03 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:23:53.60 -09:33:14.4: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:48:02.57 -08:43:07.3: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter REJECTED candidate at 15:48:02.57 -08:43:07.3: ref_mag=12.99 +/- 0.02 new_mean_mag=13.1129 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:47:34.83 -12:05:12.3: 12.34 +/- 0.02 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:41:25.81 -12:45:03.1: 13.95 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:44:04.53 -09:36:48.2: 13.03 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 15:47:34.83 -12:05:12.3: ref_mag=12.36 +/- 0.01 new_mean_mag=12.2619 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter REJECTED candidate at 15:44:04.53 -09:36:48.2: ref_mag=13.11 +/- 0.02 new_mean_mag=13.4790 delta=-0.37 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:41:25.81 -12:45:03.1: ref_mag=13.96 +/- 0.05 new_mean_mag=14.2165 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:14:14.08 -11:48:59.1: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter REJECTED candidate at 15:14:14.08 -11:48:59.1: ref_mag=13.06 +/- 0.02 new_mean_mag=13.2621 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:43:25.56 -08:38:15.4: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:32:48.53 -13:20:54.0: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:23:53.60 -09:33:14.4: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:43:25.56 -08:38:15.4: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:32:48.53 -13:20:54.0: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:23:06.92 -10:29:02.2: 13.98 +/- 0.07 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:08:35.43 -09:53:31.3: 14.28 +/- 0.09 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:25:49.40 -05:49:00.2: 13.91 +/- 0.06 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:19:24.28 -11:23:18.7: 14.13 +/- 0.08 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:41:51.08 -08:34:36.0: 14.55 +/- 0.12 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:52:58.35 -10:56:15.1: 14.45 +/- 0.14 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:40:10.00 -13:19:43.5: 14.47 +/- 0.11 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:23:06.92 -10:29:02.2: 13.81 +/- 0.06 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:08:35.43 -09:53:31.3: 14.06 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Forced photometry filter REJECTED candidate at 15:23:06.92 -10:29:02.2: ref_mag=13.89 +/- 0.05 new_mean_mag=13.7559 delta=0.13 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:19:24.28 -11:23:18.7: 14.34 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:25:49.40 -05:49:00.2: 14.13 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 15:08:35.43 -09:53:31.3: ref_mag=14.15 +/- 0.06 new_mean_mag=14.1784 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.21 +/- 0.06
Forced photometry filter REJECTED candidate at 15:19:24.28 -11:23:18.7: ref_mag=14.21 +/- 0.06 new_mean_mag=14.2196 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Forced photometry filter REJECTED candidate at 15:25:49.40 -05:49:00.2: ref_mag=14.00 +/- 0.05 new_mean_mag=14.0099 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:41:51.08 -08:34:36.0: 14.55 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.09
Forced photometry filter REJECTED candidate at 15:41:51.08 -08:34:36.0: ref_mag=14.55 +/- 0.09 new_mean_mag=14.4566 delta=0.09 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:52:58.35 -10:56:15.1: 14.71 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.11
Forced photometry filter REJECTED candidate at 15:52:58.35 -10:56:15.1: ref_mag=14.54 +/- 0.11 new_mean_mag=14.3959 delta=0.15 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:40:10.00 -13:19:43.5: 14.73 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.09
Forced photometry filter REJECTED candidate at 15:40:10.00 -13:19:43.5: ref_mag=14.56 +/- 0.09 new_mean_mag=14.5170 delta=0.04 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:28:23.67 -14:11:07.5: 14.61 +/- 0.12 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:42:17.15 -12:47:37.2: 14.55 +/- 0.12 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:53:06.27 -10:00:00.5: 14.67 +/- 0.16 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:50:28.19 -12:44:34.7: 14.57 +/- 0.14 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:19:29.97 -14:02:49.2: 15.01 +/- 0.17 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:11:07.51 -07:41:10.9: 15.20 +/- 0.19 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:28:23.67 -14:11:07.5: 14.95 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.10
Forced photometry filter REJECTED candidate at 15:28:23.67 -14:11:07.5: ref_mag=14.72 +/- 0.10 new_mean_mag=14.6216 delta=0.09 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:19:29.97 -14:02:49.2: 15.00 +/- 0.19 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:53:06.27 -10:00:00.5: 14.77 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.13
Forced photometry filter REJECTED candidate at 15:19:29.97 -14:02:49.2: ref_mag=15.01 +/- 0.13 new_mean_mag=14.6942 delta=0.31 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:50:28.19 -12:44:34.7: 14.85 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.12
Forced photometry filter REJECTED candidate at 15:53:06.27 -10:00:00.5: ref_mag=14.71 +/- 0.12 new_mean_mag=14.4278 delta=0.29 (need > 0.90)
Forced photometry reference-image weighted average: 14.67 +/- 0.11
Forced photometry filter REJECTED candidate at 15:50:28.19 -12:44:34.7: ref_mag=14.67 +/- 0.11 new_mean_mag=14.4617 delta=0.20 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:42:17.15 -12:47:37.2: 14.68 +/- 0.15 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:49:06.57 -11:32:27.4: 14.86 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.60 +/- 0.09
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:11:07.51 -07:41:10.9: 15.16 +/- 0.19 detection
Forced photometry filter REJECTED candidate at 15:42:17.15 -12:47:37.2: ref_mag=14.60 +/- 0.09 new_mean_mag=14.3658 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 15.18 +/- 0.13
Forced photometry filter REJECTED candidate at 15:11:07.51 -07:41:10.9: ref_mag=15.18 +/- 0.13 new_mean_mag=14.7851 delta=0.40 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:49:06.57 -11:32:27.4: 14.76 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.12
Forced photometry filter REJECTED candidate at 15:49:06.57 -11:32:27.4: ref_mag=14.81 +/- 0.12 new_mean_mag=14.6149 delta=0.19 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:15:16.69 -07:19:34.6: 15.45 +/- 0.23 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:49:33.90 -11:45:13.9: 15.35 +/- 0.27 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:35:24.51 -13:26:26.1: 15.26 +/- 0.24 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:50:10.03 -13:38:44.2: 14.60 +/- 0.16 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:31:47.98 -13:54:24.2: 14.75 +/- 0.14 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:34:38.03 -13:28:11.3: 15.28 +/- 0.23 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:15:16.69 -07:19:34.6: 15.33 +/- 0.21 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:49:33.90 -11:45:13.9: 14.56 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.12
Forced photometry filter REJECTED candidate at 15:49:33.90 -11:45:13.9: ref_mag=14.72 +/- 0.12 new_mean_mag=14.3760 delta=0.34 (need > 0.90)
Forced photometry reference-image weighted average: 15.38 +/- 0.15
Forced photometry filter REJECTED candidate at 15:15:16.69 -07:19:34.6: ref_mag=15.38 +/- 0.15 new_mean_mag=14.7535 delta=0.63 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:35:24.51 -13:26:26.1: 14.89 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.15
Forced photometry filter REJECTED candidate at 15:35:24.51 -13:26:26.1: ref_mag=15.03 +/- 0.15 new_mean_mag=14.6915 delta=0.34 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:50:10.03 -13:38:44.2: 14.89 +/- 0.22 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:31:47.98 -13:54:24.2: 14.76 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.13
Forced photometry filter REJECTED candidate at 15:50:10.03 -13:38:44.2: ref_mag=14.71 +/- 0.13 new_mean_mag=14.5744 delta=0.13 (need > 0.90)
Forced photometry reference-image weighted average: 14.75 +/- 0.10
Forced photometry filter REJECTED candidate at 15:31:47.98 -13:54:24.2: ref_mag=14.75 +/- 0.10 new_mean_mag=14.7517 delta=0.00 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:34:38.03 -13:28:11.3: 15.11 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.15
Forced photometry filter REJECTED candidate at 15:34:38.03 -13:28:11.3: ref_mag=15.19 +/- 0.15 new_mean_mag=14.7456 delta=0.44 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:34:59.45 -09:46:58.9: 14.84 +/- 0.15 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:34:59.45 -09:46:58.9: 14.94 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.12
Forced photometry filter REJECTED candidate at 15:34:59.45 -09:46:58.9: ref_mag=14.88 +/- 0.12 new_mean_mag=14.6473 delta=0.24 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:48:50.89 -13:33:26.8: 15.09 +/- 0.23 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:37:23.43 -13:58:16.0: 14.93 +/- 0.17 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:31:52.42 -14:15:17.8: 14.90 +/- 0.16 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:40:40.02 -10:25:24.3: 14.97 +/- 0.18 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:31:23.78 -12:41:48.8: 14.95 +/- 0.16 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:37:22.34 -14:12:40.8: 14.90 +/- 0.17 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:48:50.89 -13:33:26.8: 14.81 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.15
Forced photometry filter REJECTED candidate at 15:48:50.89 -13:33:26.8: ref_mag=14.93 +/- 0.15 new_mean_mag=14.5710 delta=0.36 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:37:23.43 -13:58:16.0: 14.76 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.12
Forced photometry filter REJECTED candidate at 15:37:23.43 -13:58:16.0: ref_mag=14.85 +/- 0.12 new_mean_mag=14.5424 delta=0.30 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:31:23.78 -12:41:48.8: 14.72 +/- 0.15 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:31:52.42 -14:15:17.8: 14.81 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.12
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:40:40.02 -10:25:24.3: 14.98 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.11
Forced photometry filter REJECTED candidate at 15:31:52.42 -14:15:17.8: ref_mag=14.86 +/- 0.12 new_mean_mag=14.7016 delta=0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:31:23.78 -12:41:48.8: ref_mag=14.83 +/- 0.11 new_mean_mag=14.6478 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 14.97 +/- 0.13
Forced photometry filter REJECTED candidate at 15:40:40.02 -10:25:24.3: ref_mag=14.97 +/- 0.13 new_mean_mag=14.5503 delta=0.42 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:37:22.34 -14:12:40.8: 14.81 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.12
Forced photometry filter REJECTED candidate at 15:37:22.34 -14:12:40.8: ref_mag=14.86 +/- 0.12 new_mean_mag=14.6487 delta=0.21 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:47:07.98 -11:04:13.1: 15.21 +/- 0.22 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:45:12.89 -11:02:16.1: 15.08 +/- 0.22 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:47:07.98 -11:04:13.1: 15.01 +/- 0.21 detection
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:37:45.56 -13:13:42.3: 15.01 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.15
Forced photometry filter REJECTED candidate at 15:47:07.98 -11:04:13.1: ref_mag=15.10 +/- 0.15 new_mean_mag=14.6299 delta=0.47 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-04-23_04-33-33_20.00sec_-5.00C_LIGHTs_0258.fits at 15:11:45.26 -07:46:50.2: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:45:12.89 -11:02:16.1: 15.30 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.17
Forced photometry filter REJECTED candidate at 15:45:12.89 -11:02:16.1: ref_mag=15.16 +/- 0.17 new_mean_mag=14.8012 delta=0.36 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:37:45.56 -13:13:42.3: 15.47 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.16
Forced photometry filter REJECTED candidate at 15:37:45.56 -13:13:42.3: ref_mag=15.14 +/- 0.16 new_mean_mag=14.6516 delta=0.48 (need > 0.90)
Forced photometry on wcs_Lib-02-Q2b1x1_2026-05-08_02-14-41_20.00sec_-5.00C_LIGHT_0275.fits at 15:11:45.26 -07:46:50.2: 15.86 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out17296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69705.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 69585_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69585_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69597_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69597_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 69598_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69598_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69606_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69606_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69608_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69608_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69611_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69611_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69626_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69626_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 69629_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69629_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 69631_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69631_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 69641_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69641_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 69643_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69643_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
**** FOUND 15:22:35.43 -08:58:21.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 69654_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69654_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
**** FOUND 15:41:17.78 -13:31:04.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 69670_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69670_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 69677_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69677_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 69680_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
Preparing report for the candidate 69680_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
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Considering the candidate 69682_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69682_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 69691_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
Preparing report for the candidate 69691_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
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Considering the candidate 69693_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69693_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 69705_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
Preparing report for the candidate 69705_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
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Considering the candidate 69710_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69710_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 69712_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69712_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 69715_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69715_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 69738_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69738_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69745_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69745_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 69771_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69771_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69773_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69773_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69782_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69782_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69812_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69812_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69820_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69820_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69834_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69834_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69845_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69845_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69857_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69857_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69866_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69866_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69870_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69870_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69875_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69875_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69883_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69883_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69894_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69894_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69898_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69898_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69919_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69919_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69928_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69928_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69933_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69933_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69937_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69937_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69940_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69940_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69942_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69942_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69951_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69951_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69952_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69952_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69972_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69972_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69978_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69978_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 69995_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 69995_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 70009_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 70009_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 70027_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 70027_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 70066_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 70066_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 70073_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 70073_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
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Considering the candidate 17296_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
Preparing report for the candidate 17296_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
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Considering the candidate 67484_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137
The candidate 67484_fd_Lib-02-Q2b1x1_2026-06-12_02-51-33_20.00sec_5.00C_LIGHT_0137 did not pass the final checks
