This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh
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 08 03.1084 2461255.6084 10.86 15:47:34.75 -27:38:36.6
344.13409 20.80728 galactic Lib Second-epoch detections are separated by 1.6" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.29 Amphitrite 1 0 1 10.9 0 -0
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 15:47:34.75 -27:38:36.6: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 15:47:34.75 -27:38:36.6: 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,2461255.6084,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.1084 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1084 2461255.6084 11.04 16:02:11.00 -21:12:57.0
351.50932 23.17313 galactic Sco Second-epoch detections are separated by 0.5" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.21 Lutetia 1 -0 1 11.4 -0 0
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:02:11.00 -21:12:57.0: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:02:11.00 -21:12:57.0: 15.29 +/- 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,2461255.6084,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.1084 11.04CV 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 08 03.1084 2461255.6084 12.86 16:03:53.13 -21:22:44.8
351.68221 22.77498 galactic Sco Second-epoch detections are separated by 1.0" and 8.8 pix
The object was found in VSX15" SSS_J160352.5-212233
Type: RRAB
# Max. Min./Amp. JD0 Period
15.270 CV Y 0.800 CV 0.583050000000
The object was found in astcheck.24 Themis 0 1 1 12.8 -0 -0
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:03:53.13 -21:22:44.8: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:03:53.13 -21:22:44.8: 15.37 +/- 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
SSS_J160352.5-212233,2461255.6084,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SSS_J160352.5-212233 20260803.1084 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1084 2461255.6084 13.24 15:52:02.83 -25:37:55.6
346.37523 21.63059 galactic Sco Second-epoch detections are separated by 3.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.674 Rachele 0 2 2 13.3 0 -0
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 15:52:02.83 -25:37:55.6: 15.17 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 15:52:02.83 -25:37:55.6: 15.14 +/- 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,2461255.6084,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.1084 13.24CV 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 08 03.1084 2461255.6084 13.29 16:26:22.01 -25:31:32.7
352.18126 16.17674 galactic Sco Second-epoch detections are separated by 0.8" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.175 Andromache 1 -1 1 13.5 0 -0
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:26:22.01 -25:31:32.7: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:26:22.01 -25:31:32.7: 15.41 +/- 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,2461255.6084,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.1084 13.29CV 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 08 03.1084 2461255.6084 12.95 16:42:51.15 -22:42:40.6
356.93369 15.11638 galactic Oph Second-epoch detections are separated by 2.1" and 8.5 pix
The object was found in VSX 1" ASASSN-V J164251.17-224239.9
Type: SR
# Max. Min./Amp. JD0 Period
13.300 V 16.200 V 2456859.00000 103.000000000000
The object was found in astcheck.1805 Dirikis 165 313 353 16.7 -0 -0
NOTE: the measured brightness disagrees with the predicted asteroid brightness, but the matched variable star above likely accounts for this object.
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:42:51.15 -22:42:40.6: 14.67 +/- 0.22 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:42:51.15 -22:42:40.6: 14.30 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.13
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
ASASSN-V J164251.17-224239.9,2461255.6084,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J164251.17-224239.9 20260803.1084 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461205.74478639 14.06.2026 05:52:19.544 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
First image: 2461205.74478639 14.06.2026 05:52:19.544 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Last image: 2461255.60868778 03.08.2026 02:36:20.624 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.15
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: 2 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7504
Objects passed selection criteria: 7488
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 5582.25
Average stars matched: 5436.75 (97.3935 %)
Memory usage VmPeak: 234020 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 2 21:38:22 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: 2461205.74478639 14.06.2026 05:52:19.544 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
First image: 2461205.74478639 14.06.2026 05:52:19.544 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Last image: 2461255.60868778 03.08.2026 02:36:20.624 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 58
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.89
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: 16 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 75054
Objects passed selection criteria: 74899
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 57882.5
Average stars matched: 55807 (96.4143 %)
Memory usage VmPeak: 493108 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 2 21:39:14 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.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-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.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: 2461255.60804635
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits exists and is non-empty
Saving wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits to local_wcs_cache/
'wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits' -> 'local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits'
wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits exists and is non-empty
Saving wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits to local_wcs_cache/
'wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits' -> 'local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits'
wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits'
wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits (1st reference image)
verification OK: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Image size: 941.3'x627.2' 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: 16:19:11.470 -25:59:09.32 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-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
Image size: 941.0'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:11.751 -26:00:00.52 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:11.470 -25:59:09.32
Second-epoch image center 16:19:11.751 -26:00:00.52
Angular distance between the image centers 0.0143 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Image size: 941.0'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:14.628 -25:59:28.69 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:11.470 -25:59:09.32
Second-epoch image center 16:19:14.628 -25:59:28.69
Angular distance between the image centers 0.0130 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 16:19:11.751 -26:00:00.52
Second-epoch second image center 16:19:14.628 -25:59:28.69
Angular distance between the image centers 0.01394 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits &> /tmp/tmp.WHBZSfaZjM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits &> /tmp/tmp.rVNxIchFYP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits &> /tmp/tmp.bhGOxI3ntt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits &> /tmp/tmp.o7aVujX0vJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.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-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits and wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits and wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat
Found non-empty wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits and wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat
The reference image (wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits) and catalog (wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat) found
'wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat' -> 'wcsmag.cat'
Read 8280 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3870 to 253.5789 deg, Dec -31.4737 to -20.0776 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 235.3870 to 253.5789 deg, Dec -31.4737 to -20.0776 deg
Loaded 8534 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): 5462 out of 5660 total matches.
Matched with Tycho-2 5660 out of 8280 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.642400
a=0.000000 b=1.000000 c=22.642400
From vast_summary.log: estimated ref. image limiting mag.: -8.15
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.49
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8280 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3870 to 253.5789 deg, Dec -31.4737 to -20.0776 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 235.3870 to 253.5789 deg, Dec -31.4737 to -20.0776 deg
Loaded 8534 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): 5462 out of 5660 total matches.
Matched with Tycho-2 5660 out of 8280 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Forced-photometry filter: calibrated wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits -> calib.txt_param_ref_wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits (aperture=5.8)
Read 8132 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.4146 to 253.5797 deg, Dec -31.4781 to -20.1157 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 235.4146 to 253.5797 deg, Dec -31.4781 to -20.1157 deg
Loaded 8515 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): 5417 out of 5611 total matches.
Matched with Tycho-2 5611 out of 8132 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
Forced-photometry filter: calibrated wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits -> calib.txt_param_ref_wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
2.3 pix Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
2.5 pix fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
2.5 pix fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Limiting magnitude estimates:
14.5 mag. Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
14.5 mag. Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
13.4 mag. fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
13.5 mag. fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.WHBZSfaZjM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.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-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits' -> 'wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat corresponding to the image wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat corresponding to the image wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=612, bad_region=0, passed=8280
Got 8280 stars (including 7650 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat
util/solve_plate_with_UCAC5 got 8280 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 4859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 8280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 8280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 8280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4859 stars left (next iteration limit 5344)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits N_match=4859 sigma_overall_arcsec=0.369 sigma_q1_arcsec=0.458 sigma_q2_arcsec=0.384 sigma_q3_arcsec=0.337 sigma_q4_arcsec=0.351 n_q1=791 n_q2=1114 n_q3=1599 n_q4=1355 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits -region wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rVNxIchFYP (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.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-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits' -> 'wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat corresponding to the image wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat corresponding to the image wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=620, bad_region=1, passed=8132
Got 8132 stars (including 7493 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat
util/solve_plate_with_UCAC5 got 8132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4907 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 4857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 8132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 8132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 8132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4856 stars left (next iteration limit 5341)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits N_match=4856 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.455 sigma_q2_arcsec=0.410 sigma_q3_arcsec=0.375 sigma_q4_arcsec=0.349 n_q1=795 n_q2=1104 n_q3=1616 n_q4=1341 worst_quadrant_to_overall_ratio=1.169
The image catalog is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits -region wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bhGOxI3ntt (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_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.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_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=415, bad_region=0, passed=2931
Got 2931 stars (including 2512 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat
util/solve_plate_with_UCAC5 got 2931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 2464 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2434 matched stars entering correct_measured_positions(), 2434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2434 matched stars entering correct_measured_positions(), 2927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 2465 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2435 matched stars entering correct_measured_positions(), 2927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 2435 matched stars entering correct_measured_positions(), 2927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 2435 stars left (next iteration limit 2677)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2435 robust_rms=11.631 arcsec worst_quadrant_rms=13.250 arcsec
SIP_REFIT: SIP order 3 trial: matched=2435 robust_rms=0.546 arcsec worst_quadrant_rms=0.570 arcsec
SIP_REFIT: SIP order 5 trial: matched=2435 robust_rms=0.398 arcsec worst_quadrant_rms=0.435 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2435 robust_rms_before=0.896 arcsec robust_rms_before_corrected=0.427 arcsec robust_rms_after=0.398 arcsec worst_quadrant_rms_before=0.519 worst_quadrant_rms_after=0.435
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
Image size: 941.1'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: 16:19:11.720 -26:00:00.84 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 2931 stars ###
'wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/correct_sextractor_wcs_catalog_usingxy2sky3405869.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.896 -> 0.398 arcsec)
WCS_QUALITY_DIAG: file=fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits N_match=2435 sigma_overall_arcsec=0.426 sigma_q1_arcsec=0.489 sigma_q2_arcsec=0.432 sigma_q3_arcsec=0.442 sigma_q4_arcsec=0.384 n_q1=378 n_q2=539 n_q3=826 n_q4=692 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits -region wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.o7aVujX0vJ (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_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.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_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=400, bad_region=0, passed=3146
Got 3146 stars (including 2742 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat
util/solve_plate_with_UCAC5 got 3146 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 2691 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2660 matched stars entering correct_measured_positions(), 2658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2660 matched stars entering correct_measured_positions(), 3143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 2692 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2659 matched stars entering correct_measured_positions(), 3143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 2659 matched stars entering correct_measured_positions(), 3143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 2659 stars left (next iteration limit 2926)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2659 robust_rms=11.830 arcsec worst_quadrant_rms=13.123 arcsec
SIP_REFIT: SIP order 3 trial: matched=2659 robust_rms=0.527 arcsec worst_quadrant_rms=0.585 arcsec
SIP_REFIT: SIP order 5 trial: matched=2659 robust_rms=0.391 arcsec worst_quadrant_rms=0.448 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2659 robust_rms_before=0.873 arcsec robust_rms_before_corrected=0.440 arcsec robust_rms_after=0.391 arcsec worst_quadrant_rms_before=0.512 worst_quadrant_rms_after=0.448
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Image size: 941.1'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: 16:19:14.605 -25:59:28.96 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3146 stars ###
'wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/correct_sextractor_wcs_catalog_usingxy2sky3405919.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.873 -> 0.391 arcsec)
WCS_QUALITY_DIAG: file=fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits N_match=2659 sigma_overall_arcsec=0.420 sigma_q1_arcsec=0.478 sigma_q2_arcsec=0.415 sigma_q3_arcsec=0.409 sigma_q4_arcsec=0.411 n_q1=419 n_q2=594 n_q3=890 n_q4=756 worst_quadrant_to_overall_ratio=1.137
The image catalog is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits -region wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits sigma_overall=0.369 worst_q_ratio=1.241
ref2=Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits sigma_overall=0.389 worst_q_ratio=1.169
new1=fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits sigma_overall=0.426 worst_q_ratio=1.146
new2=fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits sigma_overall=0.420 worst_q_ratio=1.137
reference average sigma_overall=0.379 worst_q_ratio=1.205
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164_astrometric_residuals.png (4859 matched stars from wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165_astrometric_residuals.png (4856 matched stars from wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002_astrometric_residuals.png (2435 matched stars from wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003_astrometric_residuals.png (2659 matched stars from wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits'
Preparing the HTML report for the field Sco-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20578_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 20578_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:50:11.58 -28:27:34.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03356_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 03356_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:23:35.53 -26:31:32.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Sco-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.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-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Creating symlink local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.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-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits exists and is non-empty
wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits exists and is non-empty
wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits exists and is non-empty
wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits (1st reference image)
verification OK: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Image size: 941.3'x627.2' 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: 16:19:11.470 -25:59:09.32 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-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
Image size: 941.0'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:11.751 -26:00:00.52 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:11.470 -25:59:09.32
Second-epoch image center 16:19:11.751 -26:00:00.52
Angular distance between the image centers 0.0143 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Image size: 941.0'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:14.628 -25:59:28.69 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:11.470 -25:59:09.32
Second-epoch image center 16:19:14.628 -25:59:28.69
Angular distance between the image centers 0.0130 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 16:19:11.751 -26:00:00.52
Second-epoch second image center 16:19:14.628 -25:59:28.69
Angular distance between the image centers 0.01394 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits &> /tmp/tmp.F1KLDsHAzY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits &> /tmp/tmp.gQxHMPaX3D
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits &> /tmp/tmp.ozPVTxo7m0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits &> /tmp/tmp.EmH0fiZkLn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.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-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits and wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits and wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat
Found non-empty wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits and wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat
The reference image (wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits) and catalog (wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat) found
'wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat' -> 'wcsmag.cat'
Read 83603 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3410 to 253.5804 deg, Dec -31.4744 to -20.0418 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 235.3410 to 253.5804 deg, Dec -31.4744 to -20.0418 deg
Loaded 8588 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): 6237 out of 6984 total matches.
Matched with Tycho-2 6984 out of 83603 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.490500
a=0.000000 b=1.000000 c=22.490500
From vast_summary.log: estimated ref. image limiting mag.: -7.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.60
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 83603 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3410 to 253.5804 deg, Dec -31.4744 to -20.0418 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 235.3410 to 253.5804 deg, Dec -31.4744 to -20.0418 deg
Loaded 8588 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): 6237 out of 6984 total matches.
Matched with Tycho-2 6984 out of 83603 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Forced-photometry filter: calibrated wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits -> calib.txt_param_ref_wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits (aperture=4.4)
Read 83601 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.3412 to 253.5846 deg, Dec -31.4849 to -20.0612 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 235.3412 to 253.5846 deg, Dec -31.4849 to -20.0612 deg
Loaded 8593 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): 6203 out of 6992 total matches.
Matched with Tycho-2 6992 out of 83601 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
Forced-photometry filter: calibrated wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits -> calib.txt_param_ref_wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
2.2 pix Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
2.4 pix fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
2.4 pix fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Limiting magnitude estimates:
14.6 mag. Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
14.6 mag. Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
13.5 mag. fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
13.6 mag. fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 13.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.F1KLDsHAzY (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.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-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits' -> 'wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat corresponding to the image wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat corresponding to the image wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=4520, bad_region=3, passed=83596
Got 83596 stars (including 78919 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat
util/solve_plate_with_UCAC5 got 83596 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 4875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 83575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 83575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 83575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4875 stars left (next iteration limit 5362)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits N_match=4875 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.361 sigma_q3_arcsec=0.331 sigma_q4_arcsec=0.340 n_q1=808 n_q2=1141 n_q3=1581 n_q4=1345 worst_quadrant_to_overall_ratio=1.261
The image catalog is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits -region wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.gQxHMPaX3D (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.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-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits' -> 'wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat corresponding to the image wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat corresponding to the image wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=4524, bad_region=6, passed=83586
Got 83586 stars (including 78883 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat
util/solve_plate_with_UCAC5 got 83586 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 4877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 83570 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 83570 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 83570 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4877 stars left (next iteration limit 5364)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits N_match=4877 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.438 sigma_q2_arcsec=0.392 sigma_q3_arcsec=0.354 sigma_q4_arcsec=0.343 n_q1=810 n_q2=1146 n_q3=1589 n_q4=1332 worst_quadrant_to_overall_ratio=1.160
The image catalog is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits -region wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ozPVTxo7m0 (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_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.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_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1010, bad_region=1, passed=31830
Got 31830 stars (including 30742 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat
util/solve_plate_with_UCAC5 got 31830 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 4853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 31830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 31830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 31830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4853 stars left (next iteration limit 5337)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits N_match=4853 sigma_overall_arcsec=0.453 sigma_q1_arcsec=0.524 sigma_q2_arcsec=0.428 sigma_q3_arcsec=0.439 sigma_q4_arcsec=0.431 n_q1=820 n_q2=1110 n_q3=1602 n_q4=1321 worst_quadrant_to_overall_ratio=1.157
The image catalog is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits -region wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EmH0fiZkLn (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_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.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_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1072, bad_region=1, passed=34061
Got 34061 stars (including 32914 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat
util/solve_plate_with_UCAC5 got 34061 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 4856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 34061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 34061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 34061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4853 stars left (next iteration limit 5341)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits N_match=4853 sigma_overall_arcsec=0.446 sigma_q1_arcsec=0.530 sigma_q2_arcsec=0.412 sigma_q3_arcsec=0.444 sigma_q4_arcsec=0.438 n_q1=820 n_q2=1104 n_q3=1601 n_q4=1328 worst_quadrant_to_overall_ratio=1.188
The image catalog is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits -region wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.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_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-35-25_20.00sec_-0.00C_LIGHTs_0002.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.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_2026-08-02_CI_Sco-02-Q1b1x1_213701_TTUQ1b1x1_3396379_sN6CLGDh/wcs_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003.fits
Preparing the HTML report for the field Sco-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:02:11.00 -21:12:57.0: 15.35 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:44:36.98 -25:01:15.5: 12.34 +/- 0.03 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:05:55.30 -21:45:07.1: 12.54 +/- 0.03 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 15:47:34.75 -27:38:36.6: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 15:43:56.70 -29:08:40.6: 11.30 +/- 0.01 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:08:38.67 -22:33:16.8: 12.67 +/- 0.03 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:25:44.90 -29:55:27.0: 12.38 +/- 0.04 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:23:27.83 -26:30:52.2: 12.71 +/- 0.18 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:02:11.00 -21:12:57.0: 15.29 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 15:47:34.75 -27:38:36.6: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 15:43:56.70 -29:08:40.6: 11.23 +/- 0.01 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:05:55.30 -21:45:07.1: 12.52 +/- 0.03 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:08:38.67 -22:33:16.8: 12.74 +/- 0.03 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:44:36.98 -25:01:15.5: 12.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Forced photometry filter REJECTED candidate at 15:43:56.70 -29:08:40.6: ref_mag=11.27 +/- 0.01 new_mean_mag=11.4570 delta=-0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:05:55.30 -21:45:07.1: ref_mag=12.53 +/- 0.02 new_mean_mag=12.6931 delta=-0.17 (need > 0.90)
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Forced photometry filter REJECTED candidate at 16:44:36.98 -25:01:15.5: ref_mag=12.33 +/- 0.02 new_mean_mag=12.4546 delta=-0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:08:38.67 -22:33:16.8: ref_mag=12.70 +/- 0.02 new_mean_mag=12.9159 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:25:44.90 -29:55:27.0: 12.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.03
Forced photometry filter REJECTED candidate at 16:25:44.90 -29:55:27.0: ref_mag=12.42 +/- 0.03 new_mean_mag=12.4692 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:23:27.83 -26:30:52.2: 12.73 +/- 0.19 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.13
Forced photometry filter REJECTED candidate at 16:23:27.83 -26:30:52.2: ref_mag=12.72 +/- 0.13 new_mean_mag=12.3778 delta=0.34 (need > 0.90)
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:48:12.63 -24:32:58.3: 12.45 +/- 0.04 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:03:53.13 -21:22:44.8: 15.31 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:05:42.84 -21:49:24.6: 13.11 +/- 0.05 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 15:52:02.83 -25:37:55.6: 15.17 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:26:22.01 -25:31:32.7: 15.42 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:48:12.63 -24:32:58.3: 12.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.03
Forced photometry filter REJECTED candidate at 16:48:12.63 -24:32:58.3: ref_mag=12.44 +/- 0.03 new_mean_mag=12.5944 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:03:53.13 -21:22:44.8: 15.37 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:05:42.84 -21:49:24.6: 13.03 +/- 0.05 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:26:22.01 -25:31:32.7: 15.41 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 15:52:02.83 -25:37:55.6: 15.14 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.07 +/- 0.04
Forced photometry filter REJECTED candidate at 16:05:42.84 -21:49:24.6: ref_mag=13.07 +/- 0.04 new_mean_mag=13.0276 delta=0.04 (need > 0.90)
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-19_20.00sec_0.00C_LIGHTs_0164.fits at 16:42:51.15 -22:42:40.6: 14.67 +/- 0.22 detection
Forced photometry on wcs_Sco-02-Q1b1x1_2026-06-14_00-52-59_20.00sec_-0.00C_LIGHTs_0165.fits at 16:42:51.15 -22:42:40.6: 14.30 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.13
Forced photometry filter KEPT candidate at 16:42:51.15 -22:42:40.6: ref_mag=14.42 +/- 0.13 new_mean_mag=12.9415 delta=1.48 (need > 0.90)
Adding exclusion_list_local.txt__out101790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97735.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 23s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101769_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101769_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101777_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101777_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101779_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101779_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:29:00.75 -22:19:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101782_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101782_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
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Considering the candidate 101783_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101783_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:41:07.77 -29:17:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101785_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101785_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
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Considering the candidate 101789_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101789_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:50:23.97 -28:11:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101790_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
Preparing report for the candidate 101790_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
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Considering the candidate 101792_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
Preparing report for the candidate 101792_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
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Considering the candidate 101793_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101793_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:07:39.87 -23:14:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101800_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101800_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:23:26.90 -26:31:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101804_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101804_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:19:24.62 -22:21:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101809_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101809_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
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Considering the candidate 101810_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101810_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
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Considering the candidate 101811_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101811_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:38:39.19 -30:59:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101813_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101813_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:07:42.85 -23:18:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101814_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101814_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:44:16.71 -26:00:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101816_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101816_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:16:58.39 -21:17:14.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101817_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101817_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:38:42.43 -21:20:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101818_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101818_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
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Considering the candidate 101819_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101819_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:33:54.77 -30:39:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101820_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101820_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:44:54.56 -27:27:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101821_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101821_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:44:18.15 -26:19:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101825_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101825_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:40:21.88 -21:57:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101826_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101826_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:52:23.84 -24:15:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101829_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
Preparing report for the candidate 101829_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
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Considering the candidate 101831_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101831_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
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Considering the candidate 101833_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
Preparing report for the candidate 101833_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
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Considering the candidate 101834_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101834_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:28:34.73 -25:11:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101835_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101835_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:13:51.27 -24:25:39.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101836_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
Preparing report for the candidate 101836_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
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Considering the candidate 101838_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 101838_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:22:48.92 -23:08:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70028_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 70028_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 15:44:41.16 -28:39:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29438_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 29438_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 15:55:49.87 -24:42:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22964_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 22964_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:10:26.17 -24:06:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81716_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 81716_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:31:40.83 -27:54:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31038_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 31038_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:50:25.38 -25:33:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60614_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 60614_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 15:44:59.58 -28:04:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27581_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 27581_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 15:48:10.11 -24:14:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68696_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 68696_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:05:44.65 -29:25:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42330_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 42330_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:33:47.50 -26:44:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29104_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 29104_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:36:49.84 -25:16:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100152_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 100152_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:35:42.15 -24:05:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98580_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 98580_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:29:06.06 -29:24:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97735_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
Preparing report for the candidate 97735_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
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Considering the candidate 97263_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 97263_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:18:47.40 -28:45:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95523_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 95523_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:48:48.37 -28:31:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93687_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 93687_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:11:46.02 -25:32:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12580_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 12580_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:51:52.37 -22:49:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54243_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 54243_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:50:11.56 -28:27:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18253_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 18253_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:19:41.69 -23:24:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16635_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 16635_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 15:58:15.65 -22:44:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29336_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 29336_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:17:14.64 -25:04:16.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01770_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 01770_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
**** FOUND 16:05:17.70 -20:43:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58315_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003
The candidate 58315_fd_Sco-02-Q1b1x1_2026-08-02_21-36-20_20.00sec_-0.00C_LIGHTs_0003 did not pass the final checks
