This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA
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 07 27.2198 2461248.7198 12.29 16:10:20.70 -10:09:53.8
2.15888 29.06585 galactic Sco Second-epoch detections are separated by 0.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.28 Bellona 1 0 1 12.4 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:10:20.70 -10:09:53.8: 16.73 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:10:20.70 -10:09:53.8: 16.57 +/- 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,2461248.7198,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260727.2198 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.2198 2461248.7198 12.64 16:17:47.12 -13:20:10.4
0.68663 25.65065 galactic Sco Second-epoch detections are separated by 0.3" and 5.4 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 12.7 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:17:47.12 -13:20:10.4: 16.62 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:17:47.12 -13:20:10.4: 16.44 +/- 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,2461248.7198,12.64,0.05,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 20260727.2198 12.64CV 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 07 27.2198 2461248.7198 12.68 16:26:22.84 -14:36:59.3
1.03491 23.22445 galactic Oph Second-epoch detections are separated by 0.9" and 5.5 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 12.8 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:26:22.84 -14:36:59.3: 16.70 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:26:22.84 -14:36:59.3: 16.57 +/- 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,2461248.7198,12.68,0.05,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 20260727.2198 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 27.2198 2461248.7198 13.62 15:55:10.97 -06:01:45.2
3.15645 34.58523 galactic Lib Second-epoch detections are separated by 1.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.97 Klotho -0 -1 1 13.5 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 15:55:10.97 -06:01:45.2: 16.75 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 15:55:10.97 -06:01:45.2: 16.57 +/- 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,2461248.7198,13.62,0.05,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 20260727.2198 13.62CV 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_stack5.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_stack5.fits
Last image: 2461248.72029560 27.07.2026 05:17:03.540 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: unknown
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.68
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: 22 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 16841
Objects passed selection criteria: 16768
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 10831.2
Average stars matched: 10763.5 (99.3745 %)
Memory usage VmPeak: 242736 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 27 03:25:28 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_stack5.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_stack5.fits
Last image: 2461248.72029560 27.07.2026 05:17:03.540 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
FILTER key from ref. img. header: unknown
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.45
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: 38 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 97070
Objects passed selection criteria: 96742
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 67635.8
Average stars matched: 65939.5 (97.4921 %)
Memory usage VmPeak: 1986720 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jul 26 03:08:32 CDT 2026
VaST build number 1.0rc89-174-g9b7cb13a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 27 03:34:00 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_stack5.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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_stack5.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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: 2461248.71939811
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_stack5.fits exists and is non-empty
Saving wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits to local_wcs_cache/
'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits' -> 'local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits'
wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits exists and is non-empty
Saving wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits to local_wcs_cache/
'wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits' -> 'local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits'
wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits exists and is non-empty
Saving wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits'
wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits exists and is non-empty
Saving wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_stack5.fits (1st reference image)
verification OK: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
Image size: 941.3'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:07.938 -09:59:23.16 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_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits (1st new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
Image size: 941.2'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: 16:17:15.548 -10:00:05.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:07.938 -09:59:23.16
Second-epoch image center 16:17:15.548 -10:00:05.45
Angular distance between the image centers 0.0334 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits (2nd new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
Image size: 941.2'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: 16:17:16.174 -09:59:34.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:17:07.938 -09:59:23.16
Second-epoch image center 16:17:16.174 -09:59:34.61
Angular distance between the image centers 0.0339 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 16:17:15.548 -10:00:05.45
Second-epoch second image center 16:17:16.174 -09:59:34.61
Angular distance between the image centers 0.00894 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_stack5.fits &> /tmp/tmp.WZAbAmN17C
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack4.fits &> /tmp/tmp.H1AAeFmvDr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits &> /tmp/tmp.zpTlNWbTN8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits &> /tmp/tmp.6fkUA7d21V
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat
The reference image (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits) and catalog (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat) found
'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat' -> 'wcsmag.cat'
Read 19776 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8753 to 252.4588 deg, Dec -15.6021 to -4.2252 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 235.8753 to 252.4588 deg, Dec -15.6021 to -4.2252 deg
Loaded 5263 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): 3969 out of 4278 total matches.
Matched with Tycho-2 4278 out of 19776 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.723600
a=0.000000 b=1.000000 c=22.723600
From vast_summary.log: estimated ref. image limiting mag.: -6.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 16.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 16.04
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 19776 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8753 to 252.4588 deg, Dec -15.6021 to -4.2252 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 235.8753 to 252.4588 deg, Dec -15.6021 to -4.2252 deg
Loaded 5263 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): 3969 out of 4278 total matches.
Matched with Tycho-2 4278 out of 19776 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_stack5.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_stack5.fits:
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits (aperture=6.3)
Read 17203 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8753 to 252.4982 deg, Dec -15.5992 to -4.2613 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 235.8753 to 252.4982 deg, Dec -15.5992 to -4.2613 deg
Loaded 5259 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): 3999 out of 4273 total matches.
Matched with Tycho-2 4273 out of 17203 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_stack4.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_stack4.fits:
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
2.4 pix Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
2.4 pix fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
2.4 pix fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
2.3 pix wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
2.4 pix wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
Limiting magnitude estimates:
16.0 mag. Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
15.9 mag. Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
14.0 mag. fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
14.0 mag. fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.1 (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.WZAbAmN17C (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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/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_stack5.fits 860.0
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_stack5.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_stack5.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_stack5.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.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_stack5.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits'
This WCS solution (swarp) 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_stack5.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.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_stack5.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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=1239, bad_region=0, passed=19776
Got 19776 stars (including 18515 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat
util/solve_plate_with_UCAC5 got 19776 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 19506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 19506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 19506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 973 stars left (next iteration limit 1070)
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_stack5.fits (swarp) - 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_stack5.fits N_match=973 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.393 sigma_q2_arcsec=0.445 sigma_q3_arcsec=0.372 sigma_q4_arcsec=0.424 n_q1=223 n_q2=251 n_q3=219 n_q4=280 worst_quadrant_to_overall_ratio=1.093
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.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_stack5.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.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.H1AAeFmvDr (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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/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_stack4.fits 860.0
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_stack4.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_stack4.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_stack4.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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_stack4.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_stack4.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits'
This WCS solution (swarp) 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_stack4.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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_stack4.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_stack4.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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=1070, bad_region=0, passed=17203
Got 17203 stars (including 16111 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits.wcscat
util/solve_plate_with_UCAC5 got 17203 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 16953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 16955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 16955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 973 stars left (next iteration limit 1070)
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_stack4.fits (swarp) - 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_stack4.fits N_match=973 sigma_overall_arcsec=0.410 sigma_q1_arcsec=0.426 sigma_q2_arcsec=0.415 sigma_q3_arcsec=0.423 sigma_q4_arcsec=0.391 n_q1=230 n_q2=248 n_q3=223 n_q4=272 worst_quadrant_to_overall_ratio=1.039
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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_stack4.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_stack4.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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_stack4.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.zpTlNWbTN8 (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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.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_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.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=257, bad_region=0, passed=3303
Got 3303 stars (including 3044 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat
util/solve_plate_with_UCAC5 got 3303 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 3239 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 3239 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 3239 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=967 robust_rms=8.706 arcsec
SIP_REFIT: SIP order 3 trial: matched=967 robust_rms=0.427 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=967 robust_rms_before=0.861 arcsec robust_rms_before_corrected=0.345 arcsec robust_rms_after=0.427 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.345 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits N_match=967 sigma_overall_arcsec=0.342 sigma_q1_arcsec=0.382 sigma_q2_arcsec=0.372 sigma_q3_arcsec=0.287 sigma_q4_arcsec=0.338 n_q1=230 n_q2=258 n_q3=217 n_q4=262 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits -region wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.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.6fkUA7d21V (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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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=257, bad_region=0, passed=3307
Got 3307 stars (including 3044 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat
util/solve_plate_with_UCAC5 got 3307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 3240 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 3240 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 3240 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=966 robust_rms=8.782 arcsec
SIP_REFIT: SIP order 3 trial: matched=966 robust_rms=0.391 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=966 robust_rms_before=0.854 arcsec robust_rms_before_corrected=0.335 arcsec robust_rms_after=0.391 arcsec
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best baseline 0.335 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits N_match=966 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.376 sigma_q2_arcsec=0.331 sigma_q3_arcsec=0.283 sigma_q4_arcsec=0.338 n_q1=231 n_q2=257 n_q3=214 n_q4=264 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits -region wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_stack5.fits sigma_overall=0.407 worst_q_ratio=1.093
ref2=Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits sigma_overall=0.410 worst_q_ratio=1.039
new1=fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits sigma_overall=0.342 worst_q_ratio=1.117
new2=fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits sigma_overall=0.334 worst_q_ratio=1.128
reference average sigma_overall=0.4085 worst_q_ratio=1.066
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_stack5_astrometric_residuals.png (973 matched stars from wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4_astrometric_residuals.png (973 matched stars from wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042_astrometric_residuals.png (967 matched stars from wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043_astrometric_residuals.png (966 matched stars from wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits'
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits'
Preparing the HTML report for the field Sco-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 04972_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 04972_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:21:24.45 -07:42:01.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
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_stack5.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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_stack5.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_stack5.fits
Creating symlink local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_stack5.fits exists and is non-empty
wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits exists and is non-empty
wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits exists and is non-empty
wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_stack5.fits (1st reference image)
verification OK: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
Image size: 941.3'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:07.938 -09:59:23.16 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_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits (1st new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
Image size: 941.2'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: 16:17:15.548 -10:00:05.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:07.938 -09:59:23.16
Second-epoch image center 16:17:15.548 -10:00:05.45
Angular distance between the image centers 0.0334 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits (2nd new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
Image size: 941.2'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: 16:17:16.174 -09:59:34.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:17:07.938 -09:59:23.16
Second-epoch image center 16:17:16.174 -09:59:34.61
Angular distance between the image centers 0.0339 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 16:17:15.548 -10:00:05.45
Second-epoch second image center 16:17:16.174 -09:59:34.61
Angular distance between the image centers 0.00894 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_stack5.fits &> /tmp/tmp.f9cE0kf196
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack4.fits &> /tmp/tmp.jO8F2WO5eA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits &> /tmp/tmp.apUVUN8wes
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits &> /tmp/tmp.00qgarKDx9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat
The reference image (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits) and catalog (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat) found
'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat' -> 'wcsmag.cat'
Read 111535 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8525 to 252.4884 deg, Dec -15.6149 to -4.1928 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 235.8525 to 252.4884 deg, Dec -15.6149 to -4.1928 deg
Loaded 5302 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): 3344 out of 4280 total matches.
Matched with Tycho-2 4280 out of 111535 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.615700
a=0.000000 b=1.000000 c=22.615700
From vast_summary.log: estimated ref. image limiting mag.: -6.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 16.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 16.17
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 111535 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8525 to 252.4884 deg, Dec -15.6149 to -4.1928 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 235.8525 to 252.4884 deg, Dec -15.6149 to -4.1928 deg
Loaded 5302 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): 3344 out of 4280 total matches.
Matched with Tycho-2 4280 out of 111535 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_stack5.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_stack5.fits:
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits (aperture=5.1)
Read 104115 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8754 to 252.4982 deg, Dec -15.6070 to -4.1799 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 235.8754 to 252.4982 deg, Dec -15.6070 to -4.1799 deg
Loaded 5296 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): 3416 out of 4273 total matches.
Matched with Tycho-2 4273 out of 104115 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_stack4.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_stack4.fits:
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 46 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
2.3 pix Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
2.2 pix fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
2.2 pix fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
2.3 pix wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
2.3 pix wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
Limiting magnitude estimates:
16.2 mag. Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
16.0 mag. Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
14.2 mag. fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
14.2 mag. fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.6 (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.f9cE0kf196 (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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/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_stack5.fits 860.0
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_stack5.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_stack5.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_stack5.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.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_stack5.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits'
This WCS solution (swarp) 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_stack5.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.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_stack5.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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=28, blended=10138, bad_region=0, passed=111507
Got 111507 stars (including 101247 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits.wcscat
util/solve_plate_with_UCAC5 got 111507 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 110692 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 110694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 110694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 978 stars left (next iteration limit 1075)
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_stack5.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_stack5.fits N_match=978 sigma_overall_arcsec=0.420 sigma_q1_arcsec=0.397 sigma_q2_arcsec=0.424 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.437 n_q1=236 n_q2=255 n_q3=219 n_q4=268 worst_quadrant_to_overall_ratio=1.040
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.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_stack5.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.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_stack5.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.jO8F2WO5eA (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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/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_stack4.fits 860.0
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_stack4.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_stack4.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_stack4.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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_stack4.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_stack4.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits'
This WCS solution (swarp) 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_stack4.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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_stack4.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_stack4.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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=33, blended=8823, bad_region=0, passed=104082
Got 104082 stars (including 95118 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits.wcscat
util/solve_plate_with_UCAC5 got 104082 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 103081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 103081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 103082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 977 stars left (next iteration limit 1074)
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_stack4.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_stack4.fits N_match=977 sigma_overall_arcsec=0.412 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.440 sigma_q3_arcsec=0.427 sigma_q4_arcsec=0.372 n_q1=235 n_q2=245 n_q3=225 n_q4=272 worst_quadrant_to_overall_ratio=1.067
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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_stack4.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_stack4.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.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_stack4.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.apUVUN8wes (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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.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_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.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=3, blended=703, bad_region=2, passed=28307
Got 28307 stars (including 27563 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat
util/solve_plate_with_UCAC5 got 28307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 27862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 27864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 27863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.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_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits N_match=965 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.368 sigma_q2_arcsec=0.362 sigma_q3_arcsec=0.296 sigma_q4_arcsec=0.355 n_q1=225 n_q2=254 n_q3=224 n_q4=262 worst_quadrant_to_overall_ratio=1.053
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits -region wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.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.00qgarKDx9 (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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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=3, blended=678, bad_region=2, passed=28133
Got 28133 stars (including 27413 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat
util/solve_plate_with_UCAC5 got 28133 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 27740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 27738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 27739 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits N_match=968 sigma_overall_arcsec=0.343 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.336 sigma_q3_arcsec=0.282 sigma_q4_arcsec=0.353 n_q1=226 n_q2=259 n_q3=224 n_q4=259 worst_quadrant_to_overall_ratio=1.049
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits -region wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-15-45_20.00sec_-0.00C_LIGHTs_0042.fits
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_2026-07-27_CI_Sco-01-Q1b1x1_002222_TTUQ1b1x1_2767528_kxAXwipA/wcs_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043.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_stack5.fits at 16:28:08.25 -08:49:43.8: 12.99 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:15:41.54 -05:22:21.3: 13.47 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 15:48:25.98 -05:42:37.1: 12.62 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:44:08.40 -11:03:24.4: 12.89 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 15:52:01.91 -06:16:50.5: 13.16 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:09:03.07 -05:18:17.1: 13.14 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:16:05.12 -07:56:22.6: 13.78 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:22:43.87 -12:34:01.3: 13.28 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:24:42.51 -06:32:15.1: 12.63 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:28:08.25 -08:49:43.8: 13.02 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:06:53.07 -10:11:52.2: 12.64 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:09:03.07 -05:18:17.1: 13.02 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:15:41.54 -05:22:21.3: 13.50 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:22:43.87 -12:34:01.3: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.01
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:44:08.40 -11:03:24.4: 12.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.01
Forced photometry filter REJECTED candidate at 16:28:08.25 -08:49:43.8: ref_mag=13.00 +/- 0.01 new_mean_mag=13.4307 delta=-0.43 (need > 0.90)
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Forced photometry reference-image weighted average: 13.27 +/- 0.01
Forced photometry filter REJECTED candidate at 16:15:41.54 -05:22:21.3: ref_mag=13.48 +/- 0.01 new_mean_mag=13.6890 delta=-0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:09:03.07 -05:18:17.1: ref_mag=13.08 +/- 0.01 new_mean_mag=13.4175 delta=-0.33 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:22:43.87 -12:34:01.3: ref_mag=13.27 +/- 0.01 new_mean_mag=13.5280 delta=-0.26 (need > 0.90)
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter REJECTED candidate at 16:44:08.40 -11:03:24.4: ref_mag=12.92 +/- 0.01 new_mean_mag=13.3313 delta=-0.41 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 15:48:25.98 -05:42:37.1: 12.67 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:16:05.12 -07:56:22.6: 13.87 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 15:52:01.91 -06:16:50.5: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry reference-image weighted average: 13.82 +/- 0.02
Forced photometry reference-image weighted average: 13.18 +/- 0.01
Forced photometry filter REJECTED candidate at 15:48:25.98 -05:42:37.1: ref_mag=12.64 +/- 0.01 new_mean_mag=13.0408 delta=-0.40 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:52:01.91 -06:16:50.5: ref_mag=13.18 +/- 0.01 new_mean_mag=13.2790 delta=-0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:16:05.12 -07:56:22.6: ref_mag=13.82 +/- 0.02 new_mean_mag=13.7800 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_stack4.fits at 16:24:42.51 -06:32:15.1: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter REJECTED candidate at 16:24:42.51 -06:32:15.1: ref_mag=12.62 +/- 0.01 new_mean_mag=13.0315 delta=-0.41 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:06:53.07 -10:11:52.2: 12.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter REJECTED candidate at 16:06:53.07 -10:11:52.2: ref_mag=12.66 +/- 0.01 new_mean_mag=12.9107 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:06:54.92 -07:42:02.2: 11.82 +/- 0.00 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:40:53.53 -08:17:11.5: 12.63 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:27:45.05 -08:24:36.9: 12.17 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:17:47.12 -13:20:10.4: 16.62 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:10:20.70 -10:09:53.8: 16.73 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:26:22.84 -14:36:59.3: 16.70 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:30:45.98 -09:06:25.6: 12.60 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:06:54.92 -07:42:02.2: 11.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.00
Forced photometry filter REJECTED candidate at 16:06:54.92 -07:42:02.2: ref_mag=11.82 +/- 0.00 new_mean_mag=12.0785 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:27:45.05 -08:24:36.9: 12.16 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:10:20.70 -10:09:53.8: 16.57 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:17:47.12 -13:20:10.4: 16.44 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:40:53.53 -08:17:11.5: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry filter REJECTED candidate at 16:27:45.05 -08:24:36.9: ref_mag=12.16 +/- 0.01 new_mean_mag=12.2077 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:35:39.09 -06:16:28.5: 13.15 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 16:40:53.53 -08:17:11.5: ref_mag=12.63 +/- 0.01 new_mean_mag=12.6759 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_stack4.fits at 16:26:22.84 -14:36:59.3: 16.57 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:07:19.84 -13:09:10.6: 12.99 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:35:39.09 -06:16:28.5: 13.12 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.01
Forced photometry filter REJECTED candidate at 16:35:39.09 -06:16:28.5: ref_mag=13.14 +/- 0.01 new_mean_mag=13.1571 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:30:45.98 -09:06:25.6: 12.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter REJECTED candidate at 16:30:45.98 -09:06:25.6: ref_mag=12.58 +/- 0.01 new_mean_mag=12.8311 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:17:54.49 -13:26:49.8: 13.12 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:07:19.84 -13:09:10.6: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry filter REJECTED candidate at 16:07:19.84 -13:09:10.6: ref_mag=12.99 +/- 0.01 new_mean_mag=12.9770 delta=0.01 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:26:44.93 -12:27:37.1: 13.33 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:17:54.49 -13:26:49.8: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.01
Forced photometry filter REJECTED candidate at 16:17:54.49 -13:26:49.8: ref_mag=13.09 +/- 0.01 new_mean_mag=13.1642 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:19:02.79 -07:20:00.5: 13.26 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:09:05.13 -09:39:46.6: 13.30 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:17:42.82 -06:07:14.2: 13.42 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:26:44.93 -12:27:37.1: 13.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.01
Forced photometry filter REJECTED candidate at 16:26:44.93 -12:27:37.1: ref_mag=13.34 +/- 0.01 new_mean_mag=13.3444 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:03:07.22 -05:48:09.0: 13.45 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 15:55:10.97 -06:01:45.2: 16.75 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:19:02.79 -07:20:00.5: 13.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.01
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:09:05.13 -09:39:46.6: 13.33 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 16:19:02.79 -07:20:00.5: ref_mag=13.26 +/- 0.01 new_mean_mag=13.3525 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.31 +/- 0.01
Forced photometry filter REJECTED candidate at 16:09:05.13 -09:39:46.6: ref_mag=13.31 +/- 0.01 new_mean_mag=13.4226 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:17:42.82 -06:07:14.2: 13.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.01
Forced photometry filter REJECTED candidate at 16:17:42.82 -06:07:14.2: ref_mag=13.42 +/- 0.01 new_mean_mag=13.4159 delta=0.00 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:07:17.16 -13:09:43.3: 13.55 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:03:07.22 -05:48:09.0: 13.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter REJECTED candidate at 16:03:07.22 -05:48:09.0: ref_mag=13.46 +/- 0.02 new_mean_mag=13.5146 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 15:55:10.97 -06:01:45.2: 16.57 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:21:52.01 -07:08:15.1: 13.61 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:07:17.16 -13:09:43.3: 13.61 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter REJECTED candidate at 16:07:17.16 -13:09:43.3: ref_mag=13.57 +/- 0.02 new_mean_mag=13.6369 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:11:49.88 -10:03:37.1: 13.66 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:16:52.76 -08:26:26.6: 13.67 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:21:52.01 -07:08:15.1: 13.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Forced photometry filter REJECTED candidate at 16:21:52.01 -07:08:15.1: ref_mag=13.61 +/- 0.02 new_mean_mag=13.7183 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_stack5.fits at 16:26:39.22 -08:42:22.7: 13.99 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:11:49.88 -10:03:37.1: 13.72 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.02
Forced photometry filter REJECTED candidate at 16:11:49.88 -10:03:37.1: ref_mag=13.68 +/- 0.02 new_mean_mag=13.7025 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_stack4.fits at 16:16:52.76 -08:26:26.6: 13.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.02
Forced photometry filter REJECTED candidate at 16:16:52.76 -08:26:26.6: ref_mag=13.71 +/- 0.02 new_mean_mag=13.8382 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_stack4.fits at 16:26:39.22 -08:42:22.7: 13.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.02
Forced photometry filter REJECTED candidate at 16:26:39.22 -08:42:22.7: ref_mag=13.95 +/- 0.02 new_mean_mag=14.0990 delta=-0.15 (need > 0.90)
Adding exclusion_list_local.txt__out128168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128241.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 128122_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128122_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128124_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128124_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128126_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128126_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128127_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128127_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128128_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128128_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128130_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128130_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128131_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128131_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128132_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128132_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128135_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128135_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:40:06.24 -12:33:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128137_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128137_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128138_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128138_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128141_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128141_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:42:53.78 -15:13:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128142_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128142_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 15:48:47.47 -06:31:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128143_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128143_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128165_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128165_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 15:58:10.21 -14:28:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128166_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128166_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128168_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 128168_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 128175_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128175_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128177_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 128177_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 128181_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128181_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:02:58.23 -05:49:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128185_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 128185_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 128189_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128189_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:38:16.73 -08:14:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128190_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128190_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128202_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128202_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128203_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128203_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:30:33.75 -07:30:02.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 128206_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128206_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128208_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128208_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128214_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128214_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:30:36.15 -07:29:43.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 128218_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128218_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:07:07.31 -14:03:29.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 128219_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128219_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128224_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128224_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128228_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128228_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128229_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128229_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 15:58:35.95 -05:33:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128232_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128232_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128233_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128233_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128241_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 128241_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 128243_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128243_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128245_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128245_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128246_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128246_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128248_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128248_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:11:51.99 -10:03:55.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 128251_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128251_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 128256_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 128256_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 82697_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 82697_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:44:41.81 -14:41:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51641_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 51641_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:26:54.30 -09:46:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27894_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 27894_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 16:21:24.45 -07:42:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105282_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043
The candidate 105282_fd_Sco-01-Q1b1x1_2026-07-27_00-17-03_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks