This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b
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 10.1756 2461262.6756 12.73 16:31:06.51 -05:35:37.1
9.82027 27.68705 galactic Oph Second-epoch detections are separated by 0.6" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.258 Tyche -0 0 0 12.8 0 0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:31:06.51 -05:35:37.1: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:31:06.51 -05:35:37.1: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461262.6756,12.73,0.05,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 20260810.1756 12.73CV 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 10.1756 2461262.6756 12.75 16:19:35.06 -13:51:10.3
0.55065 24.98514 galactic Sco Second-epoch detections are separated by 0.5" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.48 Doris 0 -0 0 12.9 0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:19:35.06 -13:51:10.3: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:19:35.06 -13:51:10.3: 15.78 +/- 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,2461262.6756,12.75,0.05,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 20260810.1756 12.75CV 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 10.1756 2461262.6756 13.21 16:29:20.78 -15:05:13.8
1.12003 22.37065 galactic Oph Second-epoch detections are separated by 0.5" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.119 Althaea 1 0 1 13.1 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:29:20.78 -15:05:13.8: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:29:20.78 -15:05:13.8: 15.62 +/- 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,2461262.6756,13.21,0.05,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 20260810.1756 13.21CV 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 10.1756 2461262.6756 13.96 15:57:14.34 -07:05:25.1
2.55295 33.51908 galactic Lib Second-epoch detections are separated by 0.7" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.97 Klotho -1 -0 1 13.7 0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:57:14.34 -07:05:25.1: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:57:14.34 -07:05:25.1: 15.87 +/- 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,2461262.6756,13.96,0.05,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 20260810.1756 13.96CV 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: 2461174.84044517 14.05.2026 08:10:04.463 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
First image: 2461174.84044517 14.05.2026 08:10:04.463 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Last image: 2461262.67590640 10.08.2026 04:13:08.313 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 10 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 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): 7772
Objects passed selection criteria: 7767
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 7087
Average stars matched: 6952.75 (98.1057 %)
Memory usage VmPeak: 234064 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 9 23:18:30 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: 2461174.84044517 14.05.2026 08:10:04.463 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
First image: 2461174.84044517 14.05.2026 08:10:04.463 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Last image: 2461262.67590640 10.08.2026 04:13:08.313 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 45
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 60 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): 61233
Objects passed selection criteria: 61131
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 56217.8
Average stars matched: 54498 (96.9409 %)
Memory usage VmPeak: 282132 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 9 23:21:18 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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.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: 2461262.67522657
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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits exists and is non-empty
Saving wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits to local_wcs_cache/
'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits' -> 'local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits'
wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits exists and is non-empty
Saving wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits to local_wcs_cache/
'wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits' -> 'local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits'
wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits exists and is non-empty
Saving wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits'
wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits exists and is non-empty
Saving wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (1st reference image)
verification OK: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Image size: 941.5'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: 16:17:07.919 -09:59:23.60 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-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits (1st new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
Image size: 941.1'x626.7' 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: 16:17:18.919 -09:58:10.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:07.919 -09:59:23.60
Second-epoch image center 16:17:18.919 -09:58:10.94
Angular distance between the image centers 0.0494 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits (2nd new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
Image size: 941.1'x626.7' 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: 16:17:21.730 -09:58:50.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:17:07.919 -09:59:23.60
Second-epoch image center 16:17:21.730 -09:58:50.93
Angular distance between the image centers 0.0574 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 16:17:18.919 -09:58:10.94
Second-epoch second image center 16:17:21.730 -09:58:50.93
Angular distance between the image centers 0.01601 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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits &> /tmp/tmp.6OHctZqsI9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits &> /tmp/tmp.sqWugc6Fjj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits &> /tmp/tmp.TUzzj7Z2fV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits &> /tmp/tmp.Mcyl9fLE3Z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
The reference image (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits) and catalog (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat) found
'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat' -> 'wcsmag.cat'
Read 8279 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 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 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 deg
Loaded 5209 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): 4038 out of 4209 total matches.
Matched with Tycho-2 4209 out of 8279 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.855250
a=0.000000 b=1.000000 c=22.855250
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8279 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 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 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 deg
Loaded 5209 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): 4038 out of 4209 total matches.
Matched with Tycho-2 4209 out of 8279 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (aperture=6.2)
Read 8296 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8990 to 252.4990 deg, Dec -15.6005 to -4.3251 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 235.8990 to 252.4990 deg, Dec -15.6005 to -4.3251 deg
Loaded 5223 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): 4035 out of 4212 total matches.
Matched with Tycho-2 4212 out of 8296 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
2.2 pix Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
2.3 pix fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
2.4 pix fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
Limiting magnitude estimates:
15.1 mag. Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
15.1 mag. Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
14.7 mag. fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
14.7 mag. fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.6OHctZqsI9 (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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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=513, bad_region=0, passed=8279
Got 8279 stars (including 7758 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 8279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 8279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 8279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 8279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4907 stars left (next iteration limit 5397)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits N_match=4907 sigma_overall_arcsec=0.319 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.368 sigma_q3_arcsec=0.271 sigma_q4_arcsec=0.292 n_q1=1253 n_q2=1184 n_q3=1109 n_q4=1361 worst_quadrant_to_overall_ratio=1.156
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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.sqWugc6Fjj (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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.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-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.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-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.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=538, bad_region=0, passed=8296
Got 8296 stars (including 7747 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat
util/solve_plate_with_UCAC5 got 8296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4912 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits N_match=4912 sigma_overall_arcsec=0.319 sigma_q1_arcsec=0.351 sigma_q2_arcsec=0.354 sigma_q3_arcsec=0.257 sigma_q4_arcsec=0.295 n_q1=1257 n_q2=1189 n_q3=1108 n_q4=1358 worst_quadrant_to_overall_ratio=1.112
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.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.TUzzj7Z2fV (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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.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=301, bad_region=0, passed=5995
Got 5995 stars (including 5688 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat
util/solve_plate_with_UCAC5 got 5995 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 4905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 5995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 5995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 5995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4903 stars left (next iteration limit 5394)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4903 robust_rms=9.716 arcsec worst_quadrant_rms=10.981 arcsec
SIP_REFIT: SIP order 3 trial: matched=4903 robust_rms=0.397 arcsec worst_quadrant_rms=0.407 arcsec
SIP_REFIT: SIP order 5 trial: matched=4903 robust_rms=0.303 arcsec worst_quadrant_rms=0.313 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4903 robust_rms_before=0.811 arcsec robust_rms_before_corrected=0.308 arcsec robust_rms_after=0.303 arcsec worst_quadrant_rms_before=0.325 worst_quadrant_rms_after=0.313
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.325 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits N_match=4903 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.338 sigma_q2_arcsec=0.326 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.318 n_q1=1252 n_q2=1199 n_q3=1124 n_q4=1328 worst_quadrant_to_overall_ratio=1.057
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits -region wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.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.Mcyl9fLE3Z (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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=278, bad_region=0, passed=6004
Got 6004 stars (including 5720 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat
util/solve_plate_with_UCAC5 got 6004 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 6004 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 6004 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 6004 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4907 stars left (next iteration limit 5397)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4907 robust_rms=9.590 arcsec worst_quadrant_rms=10.697 arcsec
SIP_REFIT: SIP order 3 trial: matched=4907 robust_rms=0.382 arcsec worst_quadrant_rms=0.410 arcsec
SIP_REFIT: SIP order 5 trial: matched=4907 robust_rms=0.298 arcsec worst_quadrant_rms=0.317 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4907 robust_rms_before=0.808 arcsec robust_rms_before_corrected=0.293 arcsec robust_rms_after=0.298 arcsec worst_quadrant_rms_before=0.310 worst_quadrant_rms_after=0.317
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.310 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits N_match=4907 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.291 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.308 n_q1=1258 n_q2=1198 n_q3=1124 n_q4=1327 worst_quadrant_to_overall_ratio=1.028
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits -region wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits sigma_overall=0.319 worst_q_ratio=1.156
ref2=Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits sigma_overall=0.319 worst_q_ratio=1.112
new1=fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits sigma_overall=0.320 worst_q_ratio=1.057
new2=fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits sigma_overall=0.300 worst_q_ratio=1.028
reference average sigma_overall=0.319 worst_q_ratio=1.134
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_astrometric_residuals.png (4907 matched stars from wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_astrometric_residuals.png (4912 matched stars from wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108_astrometric_residuals.png (4903 matched stars from wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109_astrometric_residuals.png (4907 matched stars from wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits'
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits'
Preparing the HTML report for the field Sco-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:13:59.46 -08:07:31.6: 11.92 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:27:45.02 -08:24:37.2: 12.15 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:13:59.46 -08:07:31.6: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter REJECTED candidate at 16:13:59.46 -08:07:31.6: ref_mag=11.92 +/- 0.01 new_mean_mag=11.8880 delta=0.03 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:27:45.02 -08:24:37.2: 12.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry filter REJECTED candidate at 16:27:45.02 -08:24:37.2: ref_mag=12.16 +/- 0.01 new_mean_mag=12.0661 delta=0.09 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20516_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 20516_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:26:54.24 -09:46:05.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20519_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 20519_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20520_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 20520_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 15:59:10.72 -14:10:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20522_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 20522_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:44:41.83 -14:41:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20525_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 20525_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02078_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 02078_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:21:24.46 -07:42:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02024_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 02024_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:45:23.15 -07:56:25.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Sco-01-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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Creating symlink local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits exists and is non-empty
wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits exists and is non-empty
wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits exists and is non-empty
wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (1st reference image)
verification OK: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Image size: 941.5'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: 16:17:07.919 -09:59:23.60 J2000 4789.000 3195.000
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The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
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# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits (1st new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
Image size: 941.1'x626.7' 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: 16:17:18.919 -09:58:10.94 J2000 4789.000 3195.000
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###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:07.919 -09:59:23.60
Second-epoch image center 16:17:18.919 -09:58:10.94
Angular distance between the image centers 0.0494 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits (2nd new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
Image size: 941.1'x626.7' 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: 16:17:21.730 -09:58:50.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:17:07.919 -09:59:23.60
Second-epoch image center 16:17:21.730 -09:58:50.93
Angular distance between the image centers 0.0574 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 16:17:18.919 -09:58:10.94
Second-epoch second image center 16:17:21.730 -09:58:50.93
Angular distance between the image centers 0.01601 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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits &> /tmp/tmp.lk5CRAjoN8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits &> /tmp/tmp.wEYiikAtSw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits &> /tmp/tmp.08hibAX3HA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits &> /tmp/tmp.i52BrYg24G
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
The reference image (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits) and catalog (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat) found
'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat' -> 'wcsmag.cat'
Read 66506 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 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 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 deg
Loaded 5306 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): 3762 out of 4283 total matches.
Matched with Tycho-2 4283 out of 66506 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.698250
a=0.000000 b=1.000000 c=22.698250
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 66506 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 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 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 deg
Loaded 5306 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): 3762 out of 4283 total matches.
Matched with Tycho-2 4283 out of 66506 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (aperture=4.5)
Read 66556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8740 to 252.4990 deg, Dec -15.6083 to -4.1791 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 235.8740 to 252.4990 deg, Dec -15.6083 to -4.1791 deg
Loaded 5298 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): 3780 out of 4279 total matches.
Matched with Tycho-2 4279 out of 66556 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
1.9 pix Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
2.2 pix fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
2.3 pix fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
Limiting magnitude estimates:
15.3 mag. Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
15.3 mag. Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
14.8 mag. fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
14.8 mag. fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.2 (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.lk5CRAjoN8 (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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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=19, blended=3301, bad_region=1, passed=66487
Got 66487 stars (including 63074 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 66487 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 4918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 66487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 66487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 66487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4918 stars left (next iteration limit 5409)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits N_match=4918 sigma_overall_arcsec=0.309 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.345 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.285 n_q1=1250 n_q2=1191 n_q3=1117 n_q4=1360 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.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.wEYiikAtSw (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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.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-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.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-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.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=27, blended=3301, bad_region=1, passed=66529
Got 66529 stars (including 63096 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat
util/solve_plate_with_UCAC5 got 66529 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 4922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 66529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4921 matched stars entering correct_measured_positions(), 66529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4921 matched stars entering correct_measured_positions(), 66529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4921 stars left (next iteration limit 5414)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits N_match=4921 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.343 sigma_q3_arcsec=0.259 sigma_q4_arcsec=0.290 n_q1=1255 n_q2=1190 n_q3=1119 n_q4=1357 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.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.08hibAX3HA (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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.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=1690, bad_region=16, passed=47315
Got 47315 stars (including 45530 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat
util/solve_plate_with_UCAC5 got 47315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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 372 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 47315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 47315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 47315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4912 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits N_match=4912 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.320 sigma_q2_arcsec=0.325 sigma_q3_arcsec=0.290 sigma_q4_arcsec=0.320 n_q1=1260 n_q2=1187 n_q3=1131 n_q4=1334 worst_quadrant_to_overall_ratio=1.027
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits -region wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.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.i52BrYg24G (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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.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=6, blended=1771, bad_region=17, passed=46122
Got 46122 stars (including 44267 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat
util/solve_plate_with_UCAC5 got 46122 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 4910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 46122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 46122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 46122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4910 stars left (next iteration limit 5401)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits N_match=4910 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.309 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.309 n_q1=1272 n_q2=1192 n_q3=1129 n_q4=1317 worst_quadrant_to_overall_ratio=1.030
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits -region wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.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-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-12-09_20.00sec_0.00C_LIGHTs_0108.fits
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.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_2026-08-09_CI_Sco-01-Q1b1x1_231343_TTUQ1b1x1_1256723_DLMG7Q8b/wcs_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109.fits
Preparing the HTML report for the field Sco-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:31:06.51 -05:35:37.1: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:28:44.40 -06:20:27.6: 13.17 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:12:11.01 -09:31:13.3: 14.53 +/- 0.09 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:44:48.64 -06:54:51.8: 13.74 +/- 0.06 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:41:45.72 -14:19:07.9: 13.63 +/- 0.06 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:19:35.06 -13:51:10.3: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:15:39.23 -07:48:06.7: 14.01 +/- 0.06 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:22:34.14 -12:26:11.4: 12.81 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:41:45.72 -14:19:07.9: 13.50 +/- 0.06 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:12:11.01 -09:31:13.3: 14.70 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Forced photometry filter REJECTED candidate at 16:41:45.72 -14:19:07.9: ref_mag=13.55 +/- 0.04 new_mean_mag=13.7079 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 14.60 +/- 0.07
Forced photometry filter REJECTED candidate at 16:12:11.01 -09:31:13.3: ref_mag=14.60 +/- 0.07 new_mean_mag=14.6927 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:19:02.82 -07:20:00.5: 13.28 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:28:44.40 -06:20:27.6: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:31:06.51 -05:35:37.1: 15.84 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 16:28:44.40 -06:20:27.6: ref_mag=13.18 +/- 0.02 new_mean_mag=13.3794 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:19:35.06 -13:51:10.3: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:44:48.64 -06:54:51.8: 13.71 +/- 0.06 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:29:20.78 -15:05:13.8: 15.62 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry filter REJECTED candidate at 16:44:48.64 -06:54:51.8: ref_mag=13.73 +/- 0.04 new_mean_mag=14.0474 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:15:39.23 -07:48:06.7: 14.09 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.04
Forced photometry filter REJECTED candidate at 16:15:39.23 -07:48:06.7: ref_mag=14.05 +/- 0.04 new_mean_mag=14.1755 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:22:34.14 -12:26:11.4: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter REJECTED candidate at 16:22:34.14 -12:26:11.4: ref_mag=12.81 +/- 0.02 new_mean_mag=12.8497 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:19:02.82 -07:20:00.5: 13.33 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter REJECTED candidate at 16:19:02.82 -07:20:00.5: ref_mag=13.30 +/- 0.03 new_mean_mag=13.2518 delta=0.05 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:29:20.78 -15:05:13.8: 15.62 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:21:51.90 -07:08:15.4: 13.66 +/- 0.05 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:32:38.42 -13:03:33.3: 13.70 +/- 0.14 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:19:59.36 -14:38:20.8: 13.40 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:45:31.49 -10:54:58.5: 13.64 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:21:51.90 -07:08:15.4: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry filter REJECTED candidate at 16:21:51.90 -07:08:15.4: ref_mag=13.64 +/- 0.03 new_mean_mag=13.4414 delta=0.20 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:19:59.36 -14:38:20.8: 13.37 +/- 0.05 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:32:38.42 -13:03:33.3: 13.64 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry reference-image weighted average: 13.67 +/- 0.09
Forced photometry filter REJECTED candidate at 16:19:59.36 -14:38:20.8: ref_mag=13.39 +/- 0.03 new_mean_mag=13.4832 delta=-0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:32:38.42 -13:03:33.3: ref_mag=13.67 +/- 0.09 new_mean_mag=13.5726 delta=0.10 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:45:31.49 -10:54:58.5: 13.65 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.05
Forced photometry filter REJECTED candidate at 16:45:31.49 -10:54:58.5: ref_mag=13.65 +/- 0.05 new_mean_mag=13.7027 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:32:05.50 -12:08:22.9: 13.95 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:07:22.39 -14:44:54.6: 13.46 +/- 0.05 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:13:17.63 -10:21:36.6: 14.02 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:32:05.50 -12:08:22.9: 13.87 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.05
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:07:22.39 -14:44:54.6: 13.43 +/- 0.05 detection
Forced photometry filter REJECTED candidate at 16:32:05.50 -12:08:22.9: ref_mag=13.91 +/- 0.05 new_mean_mag=13.7687 delta=0.14 (need > 0.90)
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter REJECTED candidate at 16:07:22.39 -14:44:54.6: ref_mag=13.44 +/- 0.03 new_mean_mag=13.7100 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:13:17.63 -10:21:36.6: 13.93 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.05
Forced photometry filter REJECTED candidate at 16:13:17.63 -10:21:36.6: ref_mag=13.97 +/- 0.05 new_mean_mag=13.8541 delta=0.12 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:57:14.34 -07:05:25.1: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:26:39.10 -08:42:28.6: 13.96 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:06:46.07 -13:55:51.3: 13.85 +/- 0.06 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:57:14.34 -07:05:25.1: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:57:38.49 -12:27:34.5: 13.92 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:26:39.10 -08:42:28.6: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter REJECTED candidate at 16:26:39.10 -08:42:28.6: ref_mag=13.93 +/- 0.04 new_mean_mag=13.9291 delta=0.00 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:06:46.07 -13:55:51.3: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.04
Forced photometry filter REJECTED candidate at 16:06:46.07 -13:55:51.3: ref_mag=13.86 +/- 0.04 new_mean_mag=14.0558 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:26:48.56 -09:50:40.7: 13.75 +/- 0.08 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:57:38.49 -12:27:34.5: 13.94 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Forced photometry filter REJECTED candidate at 15:57:38.49 -12:27:34.5: ref_mag=13.93 +/- 0.05 new_mean_mag=13.9019 delta=0.03 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:15:25.45 -11:01:28.3: 14.37 +/- 0.10 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:09:16.32 -11:32:05.9: 14.24 +/- 0.09 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:26:48.56 -09:50:40.7: 13.83 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.06
Forced photometry filter REJECTED candidate at 16:26:48.56 -09:50:40.7: ref_mag=13.79 +/- 0.06 new_mean_mag=14.0912 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:15:25.45 -11:01:28.3: 14.47 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.08
Forced photometry filter REJECTED candidate at 16:15:25.45 -11:01:28.3: ref_mag=14.41 +/- 0.08 new_mean_mag=14.2966 delta=0.12 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:56:27.11 -04:59:47.9: 15.37 +/- 0.23 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:09:16.32 -11:32:05.9: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Forced photometry filter REJECTED candidate at 16:09:16.32 -11:32:05.9: ref_mag=14.15 +/- 0.06 new_mean_mag=14.3349 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:56:27.11 -04:59:47.9: 15.15 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.15
Forced photometry filter REJECTED candidate at 15:56:27.11 -04:59:47.9: ref_mag=15.24 +/- 0.15 new_mean_mag=14.5002 delta=0.74 (need > 0.90)
Adding exclusion_list_local.txt__out82557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82691.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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: 5s
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Considering the candidate 82487_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82487_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82502_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82502_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82508_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82508_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82512_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82512_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82516_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82516_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82520_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82520_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:42:53.82 -15:13:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82548_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82548_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:46:30.61 -12:31:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82557_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
Preparing report for the candidate 82557_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
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Considering the candidate 82558_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82558_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:02:58.19 -05:49:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82560_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
Preparing report for the candidate 82560_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
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Considering the candidate 82569_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82569_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82584_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
Preparing report for the candidate 82584_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
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Considering the candidate 82587_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82587_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82598_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82598_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:33:16.77 -12:48:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82605_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82605_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82617_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82617_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82627_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82627_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82634_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82634_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82637_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82637_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:11:52.06 -10:03:55.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82638_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82638_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 15:51:51.01 -11:08:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82645_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82645_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:38:16.62 -07:06:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82648_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82648_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82651_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82651_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82680_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82680_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82691_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
Preparing report for the candidate 82691_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
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Considering the candidate 82713_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82713_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:41:48.93 -06:41:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82716_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82716_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82719_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82719_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82739_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82739_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82768_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82768_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82769_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82769_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 15:50:36.97 -11:28:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82780_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82780_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:38:14.46 -11:20:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82822_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82822_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82843_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82843_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 82851_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82851_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:26:26.50 -06:56:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82865_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 82865_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
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Considering the candidate 32325_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 32325_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:26:54.25 -09:46:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09726_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 09726_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:47:48.73 -06:46:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05644_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 05644_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:28:51.16 -05:51:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45628_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 45628_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 15:59:10.72 -14:10:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17622_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 17622_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks
**** FOUND 16:45:23.15 -07:56:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17754_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109
The candidate 17754_fd_Sco-01-Q1b1x1_2026-08-09_23-13-08_20.00sec_0.00C_LIGHTs_0109 did not pass the final checks