This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 08.1466 2461199.6466 9.88 16:05:01.10 -30:08:54.1
345.30407 16.37910 galactic Lup Second-epoch detections are separated by 2.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.29 Amphitrite 4 -1 4 9.8 -0 -0
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:05:01.10 -30:08:54.1: 14.53 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:05:01.10 -30:08:54.1: 14.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461199.6466,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260608.1466 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1466 2461199.6466 11.58 16:22:25.13 -22:09:34.9
354.19580 19.08534 galactic Sco Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.24 Themis 3 -0 3 11.8 -0 0
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:22:25.13 -22:09:34.9: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:22:25.13 -22:09:34.9: 15.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461199.6466,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260608.1466 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1466 2461199.6466 12.36 16:15:40.13 -25:15:42.0
350.67850 18.13775 galactic Sco Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.674 Rachele 3 -0 3 12.3 -0 -0
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:15:40.13 -25:15:42.0: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:15:40.13 -25:15:42.0: 15.15 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461199.6466,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260608.1466 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1466 2461199.6466 13.22 16:03:03.40 -25:53:54.6
348.09563 19.72677 galactic Sco Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.556 Phyllis 3 1 3 13.2 -0 0
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:03:03.40 -25:53:54.6: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:03:03.40 -25:53:54.6: 15.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461199.6466,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260608.1466 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1466 2461199.6466 13.68 16:02:32.17 -27:08:44.2
347.08350 18.91646 galactic Sco Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.254 Augusta 5 -1 5 13.7 -0 -0
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:02:32.17 -27:08:44.2: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:02:32.17 -27:08:44.2: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461199.6466,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260608.1466 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461147.78803603 17.04.2026 06:54:36.313 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
First image: 2461147.78803603 17.04.2026 06:54:36.313 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
Last image: 2461199.64684912 08.06.2026 03:31:17.764 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.33
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 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): 4164
Objects passed selection criteria: 4161
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 3906
Average stars matched: 3664.5 (93.8172 %)
Memory usage VmPeak: 110752 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 01:18:47 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: 2461147.78803603 17.04.2026 06:54:36.313 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
First image: 2461147.78803603 17.04.2026 06:54:36.313 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
Last image: 2461199.64684912 08.06.2026 03:31:17.764 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.98
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: 25 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): 43542
Objects passed selection criteria: 43478
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 40728.2
Average stars matched: 37704.2 (92.5752 %)
Memory usage VmPeak: 149472 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 01:21:35 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/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.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/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.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: 2461199.64630368
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits'
wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits'
wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits'
wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits (1st reference image)
verification OK: wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
Image size: 942.0'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: 16:19:12.067 -26:00:18.90 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_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
Image size: 937.7'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:19:11.628 -25:59:56.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:12.067 -26:00:18.90
Second-epoch image center 16:19:11.628 -25:59:56.90
Angular distance between the image centers 0.0063 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
Image size: 937.7'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:19:14.224 -25:59:33.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:12.067 -26:00:18.90
Second-epoch image center 16:19:14.224 -25:59:33.39
Angular distance between the image centers 0.0150 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 16:19:11.628 -25:59:56.90
Second-epoch second image center 16:19:14.224 -25:59:33.39
Angular distance between the image centers 0.01171 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/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits &> /tmp/tmp.zw329ftSE7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits &> /tmp/tmp.yQYf8UE5Vo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits &> /tmp/tmp.SdZ1HgWRH5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits &> /tmp/tmp.0GNh2WpgIZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.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_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits and wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.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_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits and wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat
Found non-empty wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits and wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat
The reference image (wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits) and catalog (wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat) found
'wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat' -> 'wcsmag.cat'
Read 5279 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3887 to 253.5849 deg, Dec -31.5354 to -20.0792 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 235.3887 to 253.5849 deg, Dec -31.5354 to -20.0792 deg
Loaded 8611 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): 4075 out of 4161 total matches.
Matched with Tycho-2 4161 out of 5279 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.386900
a=0.000000 b=1.000000 c=22.386900
From vast_summary.log: estimated ref. image limiting mag.: -8.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.06
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.06
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5279 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3887 to 253.5849 deg, Dec -31.5354 to -20.0792 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 235.3887 to 253.5849 deg, Dec -31.5354 to -20.0792 deg
Loaded 8611 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): 4075 out of 4161 total matches.
Matched with Tycho-2 4161 out of 5279 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits:
Forced-photometry filter: calibrated wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits -> calib.txt_param_ref_wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits (aperture=6.0)
Read 6303 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3727 to 253.6268 deg, Dec -31.4687 to -20.1177 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 235.3727 to 253.6268 deg, Dec -31.4687 to -20.1177 deg
Loaded 8547 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): 4618 out of 4781 total matches.
Matched with Tycho-2 4781 out of 6303 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits:
Forced-photometry filter: calibrated wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits -> calib.txt_param_ref_wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
2.1 pix Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
2.5 pix fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
2.5 pix fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
2.2 pix wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
2.1 pix wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
Limiting magnitude estimates:
14.1 mag. Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
14.2 mag. Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
13.8 mag. fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
13.8 mag. fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
All-image limiting magnitude estimate: 13.8 (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.zw329ftSE7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits' -> 'wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=390, passed=5279
Got 5279 stars (including 4876 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat
util/solve_plate_with_UCAC5 got 5279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5167 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5167 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits N_match=962 sigma_overall_arcsec=0.347 sigma_q1_arcsec=0.267 sigma_q2_arcsec=0.423 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.458 n_q1=289 n_q2=245 n_q3=272 n_q4=156 worst_quadrant_to_overall_ratio=1.321
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits -region wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.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.yQYf8UE5Vo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits' -> 'wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=573, passed=6303
Got 6303 stars (including 5717 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat
util/solve_plate_with_UCAC5 got 6303 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6163 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6163 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits N_match=959 sigma_overall_arcsec=0.461 sigma_q1_arcsec=0.405 sigma_q2_arcsec=0.478 sigma_q3_arcsec=0.403 sigma_q4_arcsec=0.650 n_q1=299 n_q2=250 n_q3=255 n_q4=155 worst_quadrant_to_overall_ratio=1.410
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits -region wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.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.SdZ1HgWRH5 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=289, passed=4885
Got 4885 stars (including 4591 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 4885 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 4760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 293 to 348 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 4759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 4758 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits N_match=957 sigma_overall_arcsec=0.625 sigma_q1_arcsec=0.482 sigma_q2_arcsec=1.096 sigma_q3_arcsec=0.464 sigma_q4_arcsec=0.896 n_q1=283 n_q2=260 n_q3=245 n_q4=169 worst_quadrant_to_overall_ratio=1.753
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits -region wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.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.0GNh2WpgIZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=300, passed=4852
Got 4852 stars (including 4548 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 4852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 348 (Dec -31.3 to -20.6)
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: 954 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 293 to 348 (Dec -31.3 to -20.6)
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: 954 matched stars entering correct_measured_positions(), 4735 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4734 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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=fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits N_match=954 sigma_overall_arcsec=0.626 sigma_q1_arcsec=0.465 sigma_q2_arcsec=1.211 sigma_q3_arcsec=0.500 sigma_q4_arcsec=0.910 n_q1=283 n_q2=264 n_q3=243 n_q4=164 worst_quadrant_to_overall_ratio=1.936
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits -region wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.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=Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits sigma_overall=0.347 worst_q_ratio=1.321
ref2=Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits sigma_overall=0.461 worst_q_ratio=1.410
new1=fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits sigma_overall=0.625 worst_q_ratio=1.753
new2=fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits sigma_overall=0.626 worst_q_ratio=1.936
reference average sigma_overall=0.404 worst_q_ratio=1.3655
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051_astrometric_residuals.png (see messages above)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits'
Preparing the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:23:22.18 -26:30:55.1: 11.46 +/- 0.05 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:05:01.10 -30:08:54.1: 14.53 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:23:22.18 -26:30:55.1: 11.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.03
Forced photometry filter REJECTED candidate at 16:23:22.18 -26:30:55.1: ref_mag=11.45 +/- 0.03 new_mean_mag=11.1075 delta=0.35 (need > 0.90)
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:05:01.10 -30:08:54.1: 14.71 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20799.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20799_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
Preparing report for the candidate 20799_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20844_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 20844_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:05:30.91 -23:28:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20858_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 20858_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20861_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 20861_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:11:41.56 -27:03:32.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20317_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 20317_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:17:39.21 -22:56:40.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:05:01.10 -30:08:54.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.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_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits exists and is non-empty
wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits exists and is non-empty
wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits exists and is non-empty
wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits (1st reference image)
verification OK: wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
Image size: 942.0'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: 16:19:12.067 -26:00:18.90 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_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
Image size: 937.7'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:19:11.628 -25:59:56.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:12.067 -26:00:18.90
Second-epoch image center 16:19:11.628 -25:59:56.90
Angular distance between the image centers 0.0063 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
Image size: 937.7'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:19:14.224 -25:59:33.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:12.067 -26:00:18.90
Second-epoch image center 16:19:14.224 -25:59:33.39
Angular distance between the image centers 0.0150 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 16:19:11.628 -25:59:56.90
Second-epoch second image center 16:19:14.224 -25:59:33.39
Angular distance between the image centers 0.01171 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/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits &> /tmp/tmp.Mo7MOk7zFU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits &> /tmp/tmp.2DTH2sehT7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits &> /tmp/tmp.jbtG9Jv4ZG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits &> /tmp/tmp.uBTXy2YkF7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.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_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits and wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.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_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits and wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat
Found non-empty wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits and wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat
The reference image (wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits) and catalog (wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat) found
'wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat' -> 'wcsmag.cat'
Read 57338 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3307 to 253.5861 deg, Dec -31.5421 to -20.0424 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 235.3307 to 253.5861 deg, Dec -31.5421 to -20.0424 deg
Loaded 8684 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): 6494 out of 7000 total matches.
Matched with Tycho-2 7000 out of 57338 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.178000
a=0.000000 b=1.000000 c=22.178000
From vast_summary.log: estimated ref. image limiting mag.: -7.98
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.20
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 57338 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3307 to 253.5861 deg, Dec -31.5421 to -20.0424 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 235.3307 to 253.5861 deg, Dec -31.5421 to -20.0424 deg
Loaded 8684 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): 6494 out of 7000 total matches.
Matched with Tycho-2 7000 out of 57338 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits:
Forced-photometry filter: calibrated wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits -> calib.txt_param_ref_wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits (aperture=4.4)
Read 69536 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3645 to 253.6286 deg, Dec -31.4708 to -20.1109 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 235.3645 to 253.6286 deg, Dec -31.4708 to -20.1109 deg
Loaded 8557 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): 6303 out of 6992 total matches.
Matched with Tycho-2 6992 out of 69536 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits:
Forced-photometry filter: calibrated wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits -> calib.txt_param_ref_wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits (aperture=4.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 33 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
2.0 pix Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
2.4 pix fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
2.4 pix fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
2.1 pix wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
2.0 pix wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
Limiting magnitude estimates:
14.2 mag. Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
14.4 mag. Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
14.0 mag. fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
14.0 mag. fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Mo7MOk7zFU (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits' -> 'wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2322, passed=57332
Got 57332 stars (including 54899 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat
util/solve_plate_with_UCAC5 got 57332 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 55902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 55899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 55899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits N_match=965 sigma_overall_arcsec=0.347 sigma_q1_arcsec=0.290 sigma_q2_arcsec=0.421 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.386 n_q1=300 n_q2=253 n_q3=262 n_q4=150 worst_quadrant_to_overall_ratio=1.213
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits -region wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.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.2DTH2sehT7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits' -> 'wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=3494, passed=69528
Got 69528 stars (including 65904 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat
util/solve_plate_with_UCAC5 got 69528 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 67452 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 67455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 67455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits N_match=966 sigma_overall_arcsec=0.457 sigma_q1_arcsec=0.374 sigma_q2_arcsec=0.493 sigma_q3_arcsec=0.431 sigma_q4_arcsec=0.638 n_q1=308 n_q2=266 n_q3=248 n_q4=144 worst_quadrant_to_overall_ratio=1.396
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits -region wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.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.jbtG9Jv4ZG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1716, passed=43349
Got 43349 stars (including 41584 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 43349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 42263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 42262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 42261 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits N_match=959 sigma_overall_arcsec=0.596 sigma_q1_arcsec=0.471 sigma_q2_arcsec=1.016 sigma_q3_arcsec=0.461 sigma_q4_arcsec=0.912 n_q1=301 n_q2=247 n_q3=247 n_q4=164 worst_quadrant_to_overall_ratio=1.705
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits -region wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.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.uBTXy2YkF7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1809, passed=43677
Got 43677 stars (including 41811 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 43677 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 42400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 42400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 42399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits N_match=960 sigma_overall_arcsec=0.636 sigma_q1_arcsec=0.479 sigma_q2_arcsec=1.055 sigma_q3_arcsec=0.528 sigma_q4_arcsec=0.982 n_q1=300 n_q2=247 n_q3=252 n_q4=161 worst_quadrant_to_overall_ratio=1.660
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits -region wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.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_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-30-30_20.00sec_4.90C_LIGHT_0050.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Sco-02-Q2b1x1_233736_TTUQ2b1x1_1167536_kUelvW5W/wcs_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051.fits
Preparing the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:22:25.13 -22:09:34.9: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:01:35.70 -25:51:20.5: 13.70 +/- 0.14 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:15:40.13 -25:15:42.0: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:03:03.40 -25:53:54.6: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:22:25.13 -22:09:34.9: 15.09 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:15:40.13 -25:15:42.0: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:01:35.70 -25:51:20.5: 13.96 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.10
Forced photometry filter REJECTED candidate at 16:01:35.70 -25:51:20.5: ref_mag=13.83 +/- 0.10 new_mean_mag=13.6143 delta=0.22 (need > 0.90)
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:36:14.84 -24:38:21.4: 14.05 +/- 0.17 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:26:34.03 -28:23:14.7: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:03:03.40 -25:53:54.6: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 15:52:01.59 -23:30:43.7: 13.83 +/- 0.15 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:02:47.40 -25:09:38.7: 13.84 +/- 0.15 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:34:38.28 -23:55:46.5: 14.31 +/- 0.21 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:03:48.09 -26:25:18.7: 13.87 +/- 0.16 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:26:34.03 -28:23:14.7: 14.19 +/- 0.17 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:36:14.84 -24:38:21.4: 14.59 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.17
Forced photometry filter REJECTED candidate at 16:26:34.03 -28:23:14.7: ref_mag=14.19 +/- 0.17 new_mean_mag=13.3938 delta=0.79 (need > 0.90)
Forced photometry reference-image weighted average: 14.24 +/- 0.14
Forced photometry filter REJECTED candidate at 16:36:14.84 -24:38:21.4: ref_mag=14.24 +/- 0.14 new_mean_mag=13.9069 delta=0.33 (need > 0.90)
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 15:58:04.81 -28:28:44.5: 13.96 +/- 0.20 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:02:47.40 -25:09:38.7: 14.44 +/- 0.21 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 15:52:01.59 -23:30:43.7: 13.65 +/- 0.10 detection
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:34:38.28 -23:55:46.5: 14.50 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.12
Forced photometry filter REJECTED candidate at 16:02:47.40 -25:09:38.7: ref_mag=14.05 +/- 0.12 new_mean_mag=13.6968 delta=0.35 (need > 0.90)
Forced photometry reference-image weighted average: 13.70 +/- 0.09
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:03:48.09 -26:25:18.7: 13.92 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.15
Forced photometry filter REJECTED candidate at 15:52:01.59 -23:30:43.7: ref_mag=13.70 +/- 0.09 new_mean_mag=13.4694 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:34:38.28 -23:55:46.5: ref_mag=14.41 +/- 0.15 new_mean_mag=13.7970 delta=0.61 (need > 0.90)
Forced photometry reference-image weighted average: 13.90 +/- 0.10
Forced photometry filter REJECTED candidate at 16:03:48.09 -26:25:18.7: ref_mag=13.90 +/- 0.10 new_mean_mag=13.7063 delta=0.19 (need > 0.90)
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 15:58:04.81 -28:28:44.5: 13.96 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.12
Forced photometry filter REJECTED candidate at 15:58:04.81 -28:28:44.5: ref_mag=13.96 +/- 0.12 new_mean_mag=13.6886 delta=0.27 (need > 0.90)
Forced photometry on wcs_Sco-02-Q2b1x1_2026-04-17_01-54-36_20.00sec_-4.90C_LIGHTs_0173.fits at 16:02:32.17 -27:08:44.2: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q2b1x1_2026-05-08_00-36-13_20.00sec_-4.90C_LIGHTs_0255.fits at 16:02:32.17 -27:08:44.2: 15.03 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out77895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78765.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 77717_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 77717_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
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Considering the candidate 77728_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 77728_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 15:53:44.68 -25:50:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77762_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 77762_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:05:01.09 -30:08:54.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 77895_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
Preparing report for the candidate 77895_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
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Considering the candidate 77942_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 77942_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:06:47.95 -21:55:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78071_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
Preparing report for the candidate 78071_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
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Considering the candidate 78104_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78104_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 15:53:56.91 -27:54:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78276_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78276_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:33:47.42 -26:44:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78311_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78311_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:18:19.41 -23:17:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78363_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78363_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:09:34.92 -27:53:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78395_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78395_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:29:28.72 -27:58:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78396_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78396_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 15:53:41.67 -25:17:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78432_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78432_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:22:48.93 -23:08:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78479_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78479_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:36:49.95 -25:16:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78521_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
Preparing report for the candidate 78521_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
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Considering the candidate 78537_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78537_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:16:58.97 -23:00:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78553_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78553_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:29:18.45 -25:52:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78619_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78619_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
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Considering the candidate 78625_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78625_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:31:43.20 -26:02:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78649_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78649_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:37:22.17 -26:57:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78681_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78681_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:32:18.23 -22:11:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78695_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78695_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 15:52:07.70 -22:12:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78697_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78697_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
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Considering the candidate 78700_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78700_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
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Considering the candidate 78716_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78716_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
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Considering the candidate 78722_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78722_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
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Considering the candidate 78728_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78728_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
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Considering the candidate 78734_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 78734_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
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Considering the candidate 78765_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
Preparing report for the candidate 78765_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
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Considering the candidate 67834_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 67834_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 15:55:38.36 -29:15:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25529_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 25529_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:11:41.59 -27:03:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67544_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 67544_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
**** FOUND 16:11:03.42 -25:39:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52502_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051
The candidate 52502_fd_Sco-02-Q2b1x1_2026-06-07_22-31-17_20.00sec_5.00C_LIGHT_0051 did not pass the final checks
