This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV
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 05 28.1304 2461188.6304 10.56 07:07:42.22 +45:31:44.1
171.69915 21.69125 galactic Lyn Second-epoch detections are separated by 0.6" and 3.3 pix
The object was found in VSX 3" NSVS J0707423+453147
Type: L:
# Max. Min./Amp. JD0 Period
9.791 R1 Y 0.340 R1 51.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 07:07:42.22 +45:31:44.1: 11.51 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:07:42.22 +45:31:44.1: 11.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
NSVS J0707423+453147,2461188.6304,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0707423+453147 20260528.1304 10.56CV 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 05 28.1304 2461188.6304 10.14 06:34:13.87 +45:57:59.5
169.17771 16.34505 galactic Aur Second-epoch detections are separated by 0.2" and 3.1 pix
The object was found in VSX 3" V0521 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
11.000 V 11.700 V
The object was not found in astcheck.
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 06:34:13.87 +45:57:59.5: 11.07 +/- 0.00 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:34:13.87 +45:57:59.5: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.07 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
V0521 Aur,2461188.6304,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0521 Aur 20260528.1304 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.1304 2461188.6304 10.66 07:10:45.13 +47:02:50.0
170.29120 22.63057 galactic Lyn Second-epoch detections are separated by 0.5" and 3.4 pix
The object was found in VSX 0" NSVS 4660211
Type: L
# Max. Min./Amp. JD0 Period
9.600 R1 10.000 R1
The object was not found in astcheck.
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 07:10:45.13 +47:02:50.0: 11.62 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:10:45.13 +47:02:50.0: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
NSVS 4660211,2461188.6304,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 4660211 20260528.1304 10.66CV 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 05 28.1304 2461188.6304 11.41 07:10:07.20 +48:11:26.3
169.06729 22.84170 galactic Lyn Second-epoch detections are separated by 0.6" and 3.3 pix
The object was found in VSX 1" NSVS J0710072+481127
Type: L:
# Max. Min./Amp. JD0 Period
10.477 R1 Y 0.445 R1 213.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 07:10:07.20 +48:11:26.3: 12.44 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:10:07.20 +48:11:26.3: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
NSVS J0710072+481127,2461188.6304,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0710072+481127 20260528.1304 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 28.1304 2461188.6304 9.42 06:58:01.24 +45:10:08.0
171.50290 19.96207 galactic Lyn Second-epoch detections are separated by 0.1" and 3.2 pix
The object was found in VSX 1" NSV 17243
Type: VAR:
# Max. Min./Amp. JD0 Period
9.900 V 10.500 V M7
The object was not found in astcheck.
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 06:58:01.24 +45:10:08.0: 10.36 +/- 0.00 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:58:01.24 +45:10:08.0: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.38 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 17243,2461188.6304,9.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 17243 20260528.1304 9.42CV 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: 2461058.75704698 18.01.2026 06:09:58.859 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
First image: 2461058.75704698 18.01.2026 06:09:58.859 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
Last image: 2461188.63060110 28.05.2026 03:07:53.935 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 7 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): 16154
Objects passed selection criteria: 16051
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 10846.2
Average stars matched: 10539.8 (97.1741 %)
Memory usage VmPeak: 120812 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed May 27 22:11:47 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: 2461058.75704698 18.01.2026 06:09:58.859 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
First image: 2461058.75704698 18.01.2026 06:09:58.859 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
Last image: 2461188.63060110 28.05.2026 03:07:53.935 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 64
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.21
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 18 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): 99624
Objects passed selection criteria: 99330
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 65432.2
Average stars matched: 62714.8 (95.8468 %)
Memory usage VmPeak: 2717792 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed May 27 22:14:35 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
SExtractor catalog cache: saved Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat to cache
SExtractor catalog cache: saved Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.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: 2461188.63015069
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits exists and is non-empty
Saving wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits to local_wcs_cache/
'wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits' -> 'local_wcs_cache/wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits'
wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits exists and is non-empty
Saving wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits to local_wcs_cache/
'wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits' -> 'local_wcs_cache/wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits'
wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits exists and is non-empty
Saving wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits to local_wcs_cache/
'wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits' -> 'local_wcs_cache/wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits'
wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits exists and is non-empty
Saving wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits to local_wcs_cache/
'wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits' -> 'local_wcs_cache/wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits (1st reference image)
verification OK: wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:12:00.639 +46:00:00.73 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_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits (1st new image)
verification OK: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
Image size: 941.4'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 07:12:12.702 +46:00:37.55 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:12:00.639 +46:00:00.73
Second-epoch image center 07:12:12.702 +46:00:37.55
Angular distance between the image centers 0.0364 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits (2nd new image)
verification OK: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
Image size: 941.4'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 07:12:13.738 +46:00:53.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:12:00.639 +46:00:00.73
Second-epoch image center 07:12:13.738 +46:00:53.93
Angular distance between the image centers 0.0407 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 07:12:12.702 +46:00:37.55
Second-epoch second image center 07:12:13.738 +46:00:53.93
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/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits &> /tmp/tmp.51Wo5r60FS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits &> /tmp/tmp.yf3jSwepeM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits &> /tmp/tmp.5d7JjFBreC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits &> /tmp/tmp.jVAZx6L02w
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.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_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat
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_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat
Found non-empty wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat
The reference image (wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits) and catalog (wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat) found
'wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat' -> 'wcsmag.cat'
Read 16932 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2429 to 119.8616 deg, Dec +39.8318 to +51.4024 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 95.2429 to 119.8616 deg, Dec 39.8318 to 51.4024 deg
Loaded 8892 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): 5924 out of 6500 total matches.
Matched with Tycho-2 6500 out of 16932 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.920150
a=0.000000 b=1.000000 c=22.920150
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 16932 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2429 to 119.8616 deg, Dec +39.8318 to +51.4024 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 95.2429 to 119.8616 deg, Dec 39.8318 to 51.4024 deg
Loaded 8892 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): 5924 out of 6500 total matches.
Matched with Tycho-2 6500 out of 16932 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits:
Forced-photometry filter: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits -> calib.txt_param_ref_wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits (aperture=6.3)
Read 16801 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2070 to 119.8616 deg, Dec +39.8318 to +51.4024 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 95.2070 to 119.8616 deg, Dec 39.8318 to 51.4024 deg
Loaded 8907 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): 5898 out of 6500 total matches.
Matched with Tycho-2 6500 out of 16801 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits:
Forced-photometry filter: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits -> calib.txt_param_ref_wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
2.1 pix Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
4.6 pix fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
4.6 pix fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
2.1 pix wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
2.1 pix wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Limiting magnitude estimates:
15.4 mag. Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
15.4 mag. Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
13.4 mag. fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
13.4 mag. fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 11.0 (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.51Wo5r60FS (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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits' -> 'wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
WCS-calibrated image found: wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
Checking if the catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
WCS catalog name: wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1394, passed=16932
Got 16932 stars (including 15519 good ones) from the SExtractor catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat
util/solve_plate_with_UCAC5 got 16932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 16721 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 16717 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 16717 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits N_match=954 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.426 sigma_q2_arcsec=0.302 sigma_q3_arcsec=0.346 sigma_q4_arcsec=0.315 n_q1=255 n_q2=230 n_q3=242 n_q4=227 worst_quadrant_to_overall_ratio=1.216
The image catalog is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits -region wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yf3jSwepeM (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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_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/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits' -> 'wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS-calibrated image found: wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Checking if the catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS catalog name: wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1405, passed=16801
Got 16801 stars (including 15373 good ones) from the SExtractor catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat
util/solve_plate_with_UCAC5 got 16801 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 16494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 16494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 16494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits N_match=956 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.349 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.321 n_q1=253 n_q2=233 n_q3=240 n_q4=230 worst_quadrant_to_overall_ratio=1.162
The image catalog is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits -region wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5d7JjFBreC (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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
Checking if the catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
WCS catalog name: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=274, passed=4999
Got 4999 stars (including 4722 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat
util/solve_plate_with_UCAC5 got 4999 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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits N_match=936 sigma_overall_arcsec=0.492 sigma_q1_arcsec=0.481 sigma_q2_arcsec=0.768 sigma_q3_arcsec=0.334 sigma_q4_arcsec=0.487 n_q1=245 n_q2=222 n_q3=237 n_q4=232 worst_quadrant_to_overall_ratio=1.562
The image catalog is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits -region wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.jVAZx6L02w (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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
Checking if the catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
WCS catalog name: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=246, passed=4954
Got 4954 stars (including 4705 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat
util/solve_plate_with_UCAC5 got 4954 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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 4866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits N_match=939 sigma_overall_arcsec=0.505 sigma_q1_arcsec=0.497 sigma_q2_arcsec=0.759 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.531 n_q1=250 n_q2=218 n_q3=236 n_q4=235 worst_quadrant_to_overall_ratio=1.502
The image catalog is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits -region wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat.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=Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits sigma_overall=0.350 worst_q_ratio=1.216
ref2=Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits sigma_overall=0.368 worst_q_ratio=1.162
new1=fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits sigma_overall=0.492 worst_q_ratio=1.562
new2=fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits sigma_overall=0.505 worst_q_ratio=1.502
reference average sigma_overall=0.359 worst_q_ratio=1.189
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257_astrometric_residuals.png (954 matched stars from wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258_astrometric_residuals.png (956 matched stars from wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032_astrometric_residuals.png (936 matched stars from wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033_astrometric_residuals.png (939 matched stars from wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits'
Saving fully-calibrated image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits'
Preparing the HTML report for the field Lyn-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 07:07:42.22 +45:31:44.1: 11.51 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 06:34:13.87 +45:57:59.5: 11.07 +/- 0.00 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:07:42.22 +45:31:44.1: 11.49 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:34:13.87 +45:57:59.5: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.50 +/- 0.00
Forced photometry reference-image weighted average: 11.07 +/- 0.00
Forced photometry filter KEPT candidate at 07:07:42.22 +45:31:44.1: ref_mag=11.50 +/- 0.00 new_mean_mag=10.5656 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 06:34:13.87 +45:57:59.5: ref_mag=11.07 +/- 0.00 new_mean_mag=10.1473 delta=0.92 (need > 0.90)
Adding exclusion_list_local.txt__out08153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10006.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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
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Considering the candidate 21030_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 21030_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:09.55 +45:48:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20431_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 20431_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:41:13.00 +44:09:59.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08153_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
Preparing report for the candidate 08153_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03227_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 03227_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:20:33.61 +42:35:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09520_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 09520_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:32.00 +46:06:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10987_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 10987_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:20.98 +47:24:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10006_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
Preparing report for the candidate 10006_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05051_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 05051_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:25:43.64 +43:43:41.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Lyn-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:07:42.22 +45:31:44.1
06:34:13.87 +45:57:59.5
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
SExtractor catalog cache: saved Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat to cache
SExtractor catalog cache: saved Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
Creating symlink local_wcs_cache/wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.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_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits exists and is non-empty
wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits exists and is non-empty
wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits exists and is non-empty
wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits (1st reference image)
verification OK: wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:12:00.639 +46:00:00.73 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_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits (1st new image)
verification OK: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
Image size: 941.4'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 07:12:12.702 +46:00:37.55 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:12:00.639 +46:00:00.73
Second-epoch image center 07:12:12.702 +46:00:37.55
Angular distance between the image centers 0.0364 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits (2nd new image)
verification OK: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
Image size: 941.4'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 07:12:13.738 +46:00:53.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:12:00.639 +46:00:00.73
Second-epoch image center 07:12:13.738 +46:00:53.93
Angular distance between the image centers 0.0407 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 07:12:12.702 +46:00:37.55
Second-epoch second image center 07:12:13.738 +46:00:53.93
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/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits &> /tmp/tmp.PWL9tjkfZf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits &> /tmp/tmp.M3JuZjQTrp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits &> /tmp/tmp.u6afBgblrK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits &> /tmp/tmp.kRnMVvpYyi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.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_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat
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_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat
Found non-empty wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat
The reference image (wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits) and catalog (wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat) found
'wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat' -> 'wcsmag.cat'
Read 107702 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2072 to 119.9274 deg, Dec +39.7760 to +51.4130 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 95.2072 to 119.9274 deg, Dec 39.7760 to 51.4130 deg
Loaded 8998 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): 5112 out of 6518 total matches.
Matched with Tycho-2 6518 out of 107702 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.793400
a=0.000000 b=1.000000 c=22.793400
From vast_summary.log: estimated ref. image limiting mag.: -7.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 107702 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2072 to 119.9274 deg, Dec +39.7760 to +51.4130 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 95.2072 to 119.9274 deg, Dec 39.7760 to 51.4130 deg
Loaded 8998 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): 5112 out of 6518 total matches.
Matched with Tycho-2 6518 out of 107702 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits:
Forced-photometry filter: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits -> calib.txt_param_ref_wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits (aperture=4.8)
Read 108521 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2070 to 119.8820 deg, Dec +39.7742 to +51.4072 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 95.2070 to 119.8820 deg, Dec 39.7742 to 51.4072 deg
Loaded 8990 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): 5101 out of 6522 total matches.
Matched with Tycho-2 6522 out of 108521 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits:
Forced-photometry filter: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits -> calib.txt_param_ref_wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 56 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
1.9 pix Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
4.0 pix fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
4.0 pix fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
2.0 pix wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
1.9 pix wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Limiting magnitude estimates:
15.6 mag. Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
15.6 mag. Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
13.5 mag. fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
13.5 mag. fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 12.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.PWL9tjkfZf (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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits' -> 'wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
WCS-calibrated image found: wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
Checking if the catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits
WCS catalog name: wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=9420, passed=107649
Got 107649 stars (including 98035 good ones) from the SExtractor catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat
util/solve_plate_with_UCAC5 got 107649 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 105338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 105340 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 105342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits N_match=953 sigma_overall_arcsec=0.364 sigma_q1_arcsec=0.426 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.304 sigma_q4_arcsec=0.331 n_q1=253 n_q2=225 n_q3=240 n_q4=235 worst_quadrant_to_overall_ratio=1.168
The image catalog is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits -region wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.M3JuZjQTrp (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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_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/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits' -> 'wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS-calibrated image found: wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Checking if the catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS catalog name: wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=9545, passed=108488
Got 108488 stars (including 98737 good ones) from the SExtractor catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat
util/solve_plate_with_UCAC5 got 108488 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 106518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 106518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 106518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits N_match=958 sigma_overall_arcsec=0.387 sigma_q1_arcsec=0.423 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.370 sigma_q4_arcsec=0.360 n_q1=259 n_q2=227 n_q3=242 n_q4=230 worst_quadrant_to_overall_ratio=1.092
The image catalog is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits -region wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.u6afBgblrK (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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
Checking if the catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
WCS catalog name: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=968, passed=23800
Got 23800 stars (including 22814 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat
util/solve_plate_with_UCAC5 got 23800 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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 23449 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 23449 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 23449 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits N_match=937 sigma_overall_arcsec=0.496 sigma_q1_arcsec=0.519 sigma_q2_arcsec=0.792 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.512 n_q1=256 n_q2=214 n_q3=239 n_q4=228 worst_quadrant_to_overall_ratio=1.596
The image catalog is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits -region wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kRnMVvpYyi (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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
Checking if the catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
WCS catalog name: wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=972, passed=23782
Got 23782 stars (including 22796 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat
util/solve_plate_with_UCAC5 got 23782 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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 23461 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 23459 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 23459 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits N_match=938 sigma_overall_arcsec=0.517 sigma_q1_arcsec=0.530 sigma_q2_arcsec=0.752 sigma_q3_arcsec=0.364 sigma_q4_arcsec=0.542 n_q1=256 n_q2=213 n_q3=238 n_q4=231 worst_quadrant_to_overall_ratio=1.453
The image catalog is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits -region wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits.cat.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_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-15_20.00sec_-0.00C_LIGHTs_0032.fits
Saving fully-calibrated image wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.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_2026-05-27_CI_Lyn-03-Q1b1x1_220928_TTUQ1b1x1_3520807_rINsyVSV/wcs_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033.fits
Preparing the HTML report for the field Lyn-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 07:20:17.64 +50:29:34.1: 12.56 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 06:53:05.37 +50:05:55.9: 12.52 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 07:20:57.96 +41:38:31.8: 12.78 +/- 0.02 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 07:28:31.37 +47:55:14.8: 12.51 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:20:57.96 +41:38:31.8: 12.89 +/- 0.02 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:20:17.64 +50:29:34.1: 12.60 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:53:05.37 +50:05:55.9: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter REJECTED candidate at 07:20:57.96 +41:38:31.8: ref_mag=12.83 +/- 0.01 new_mean_mag=13.0760 delta=-0.25 (need > 0.90)
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter REJECTED candidate at 07:20:17.64 +50:29:34.1: ref_mag=12.58 +/- 0.01 new_mean_mag=12.4932 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:53:05.37 +50:05:55.9: ref_mag=12.54 +/- 0.01 new_mean_mag=12.4521 delta=0.09 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:28:31.37 +47:55:14.8: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter REJECTED candidate at 07:28:31.37 +47:55:14.8: ref_mag=12.51 +/- 0.01 new_mean_mag=12.3045 delta=0.21 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 07:10:07.20 +48:11:26.3: 12.44 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 07:10:45.13 +47:02:50.0: 11.62 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-09-58_20.00sec_-15.00C_LIGHT_0257.fits at 06:58:01.24 +45:10:08.0: 10.36 +/- 0.00 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:10:45.13 +47:02:50.0: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.00
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:10:07.20 +48:11:26.3: 12.44 +/- 0.01 detection
Forced photometry filter KEPT candidate at 07:10:45.13 +47:02:50.0: ref_mag=11.61 +/- 0.00 new_mean_mag=10.6599 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter KEPT candidate at 07:10:07.20 +48:11:26.3: ref_mag=12.44 +/- 0.01 new_mean_mag=11.4135 delta=1.03 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:58:01.24 +45:10:08.0: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.38 +/- 0.00
Forced photometry filter KEPT candidate at 06:58:01.24 +45:10:08.0: ref_mag=10.38 +/- 0.00 new_mean_mag=9.4165 delta=0.96 (need > 0.90)
Adding exclusion_list_local.txt__out100047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65746.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 127016_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127016_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
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Considering the candidate 127032_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127032_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
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Considering the candidate 127034_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127034_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
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Considering the candidate 127196_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127196_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 127231_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127231_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 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 127320_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127320_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 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 127422_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127422_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 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 127496_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127496_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:58:27.22 +48:41:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127611_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127611_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:29:46.49 +49:40:28.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 127625_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127625_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:02:40.49 +51:09:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127727_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127727_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
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Considering the candidate 127767_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127767_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:50:16.39 +45:47:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127811_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127811_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 127812_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127812_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:57:28.92 +45:04:32.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 127855_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127855_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:25.41 +45:13:43.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 127859_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127859_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:57:40.05 +45:07:15.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 127935_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127935_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:26.15 +49:26:13.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 127969_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127969_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:43.09 +47:15:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127973_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 127973_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:29:50.54 +46:40:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128151_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 128151_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:49.22 +45:24:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128172_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 128172_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:23.46 +43:44:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128197_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 128197_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:24:38.36 +41:59:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128235_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 128235_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:27:26.38 +45:40:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128242_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 128242_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:54.18 +41:54:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128295_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 128295_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 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 128354_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 128354_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 128372_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 128372_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 128376_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 128376_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 59874_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 59874_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:32.00 +46:06:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61132_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 61132_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:55:21.29 +46:17:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63377_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 63377_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:34:13.87 +45:57:59.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 107385_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 107385_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:20.93 +47:24:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80525_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 80525_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:36.22 +50:10:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49964_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 49964_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:42.22 +45:31:44.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 17190_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 17190_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:20:33.61 +42:35:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65746_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
Preparing report for the candidate 65746_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
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Considering the candidate 100047_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
Preparing report for the candidate 100047_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
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Considering the candidate 47826_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
Preparing report for the candidate 47826_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
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Considering the candidate 51895_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 51895_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:09.54 +45:48:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42348_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 42348_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:41:12.99 +44:09:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29055_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 29055_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:25:43.61 +43:43:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75617_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 75617_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:50.11 +47:14:19.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 44423_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 44423_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:17.17 +45:13:45.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 63565_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 63565_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:56:56.12 +46:42:18.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 46466_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 46466_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:57:37.39 +45:05:43.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 59248_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 59248_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:56:32.37 +46:16:29.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 51251_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 51251_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:28:11.38 +45:59:26.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 87572_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 87572_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:31.80 +49:27:50.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 90688_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 90688_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:26:42.43 +49:12:37.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 89314_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 89314_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:39.97 +48:47:21.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 86296_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 86296_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:29:55.99 +49:40:16.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 33241_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 33241_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:44.68 +43:34:48.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 44232_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 44232_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:43:05.11 +44:31:30.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105083_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 105083_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:30:03.12 +46:41:08.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 12702_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 12702_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:50:45.99 +41:46:52.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 23869_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033
The candidate 23869_fd_Lyn-03-Q1b1x1_2026-05-27_22-07-53_20.00sec_-0.00C_LIGHTs_0033 did not pass the final checks