This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr
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 09 08.1517 2461291.6517 12.68 16:31:14.90 -13:45:44.5
2.55704 22.82576 galactic Oph Second-epoch detections are separated by 0.7" and 6.7 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 13.0 0 -0
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:31:14.90 -13:45:44.5: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:31:14.90 -13:45:44.5: 15.70 +/- 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,2461291.6517,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260908.1517 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 09 08.1517 2461291.6517 13.69 16:26:14.14 -07:19:33.5
7.43383 27.67438 galactic Oph Second-epoch detections are separated by 1.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.660 Crescentia 1 -1 1 13.8 -0 -0
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:26:14.14 -07:19:33.5: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:26:14.14 -07:19:33.5: 15.81 +/- 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,2461291.6517,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260908.1517 13.69CV 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 09 08.1517 2461291.6517 13.99 16:13:37.92 -06:02:02.3
6.50136 30.96103 galactic Oph Second-epoch detections are separated by 2.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.304 Olga 0 1 1 14.4 0 -0
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:13:37.92 -06:02:02.3: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:13:37.92 -06:02:02.3: 16.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461291.6517,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260908.1517 13.99CV 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 09 08.1517 2461291.6517 12.27 16:18:28.01 -08:11:45.1
5.34105 28.70288 galactic Oph Second-epoch detections are separated by 0.4" and 6.7 pix
The object was found in VSX 1" ASAS J161828-0811.8
Type: M
# Max. Min./Amp. JD0 Period
10.700 V 14.200 V 2452719.00000 335.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:18:28.01 -08:11:45.1: 13.20 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:18:28.01 -08:11:45.1: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
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
ASAS J161828-0811.8,2461291.6517,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J161828-0811.8 20260908.1517 12.27CV 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-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
First image: 2461174.84044517 14.05.2026 08:10:04.463 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Last image: 2461291.65193833 08.09.2026 03:38:37.472 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
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: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 6087
Objects passed selection criteria: 6077
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 5192.25
Average stars matched: 5054.25 (97.3422 %)
Memory usage VmPeak: 233096 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 22:55:37 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-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
First image: 2461174.84044517 14.05.2026 08:10:04.463 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Last image: 2461291.65193833 08.09.2026 03:38:37.472 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 41
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.37
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: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 50228
Objects passed selection criteria: 50120
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 42484.5
Average stars matched: 40959.5 (96.4105 %)
Memory usage VmPeak: 275540 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 22:59:32 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
SExtractor catalog cache: saved Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.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: 2461291.65139890
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits exists and is non-empty
wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits exists and is non-empty
wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits exists and is non-empty
wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (1st reference image)
verification OK: wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:07.919 -09:59:23.60 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits (1st new image)
verification OK: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:17:07.915 -10:00:04.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:07.919 -09:59:23.60
Second-epoch image center 16:17:07.915 -10:00:04.22
Angular distance between the image centers 0.0113 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits (2nd new image)
verification OK: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:17:06.452 -09:59:31.35 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:17:07.919 -09:59:23.60
Second-epoch image center 16:17:06.452 -09:59:31.35
Angular distance between the image centers 0.0064 deg.
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# 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 16:17:07.915 -10:00:04.22
Second-epoch second image center 16:17:06.452 -09:59:31.35
Angular distance between the image centers 0.01093 deg.
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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-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits &> /tmp/tmp.Ujz7ZvKwxv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits &> /tmp/tmp.T7BEAyZbcR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits &> /tmp/tmp.4SHi7bxduV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits &> /tmp/tmp.3tu4ZNh1mt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
'tns_transients_list.txt' -> '../tns_transients_list.txt'
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-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
Found non-empty wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
The reference image (wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits) and catalog (wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat) found
'wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat' -> 'wcsmag.cat'
Read 8279 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 deg
Loaded 5209 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4038 out of 4209 total matches.
Matched with Tycho-2 4209 out of 8279 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.848950
a=0.000000 b=1.000000 c=22.848950
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.10
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.10
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8279 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 deg
Loaded 5209 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4038 out of 4209 total matches.
Matched with Tycho-2 4209 out of 8279 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -> calib.txt_param_ref_wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (aperture=6.1)
Read 8296 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8990 to 252.4990 deg, Dec -15.6005 to -4.3251 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8990 to 252.4990 deg, Dec -15.6005 to -4.3251 deg
Loaded 5223 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4035 out of 4212 total matches.
Matched with Tycho-2 4212 out of 8296 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -> calib.txt_param_ref_wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
2.2 pix Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
2.5 pix fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
2.5 pix fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
Limiting magnitude estimates:
15.1 mag. Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
15.1 mag. Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
14.3 mag. fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
14.3 mag. fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.6 (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
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.Ujz7ZvKwxv (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits' -> 'wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS-calibrated image found: wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Checking if the catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS catalog name: wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=513, bad_region=1847, passed=8279
Got 8279 stars (including 6024 good ones) from the SExtractor catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 8279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 4906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 6859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 6859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 6859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4906 stars left (next iteration limit 5396)
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-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits N_match=4906 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.437 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.310 n_q1=1586 n_q2=886 n_q3=1462 n_q4=972 worst_quadrant_to_overall_ratio=1.338
The image catalog is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -region wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.T7BEAyZbcR (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits' -> 'wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS-calibrated image found: wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Checking if the catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS catalog name: wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=538, bad_region=1845, passed=8296
Got 8296 stars (including 6022 good ones) from the SExtractor catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat
util/solve_plate_with_UCAC5 got 8296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 6865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 6865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 6865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4906 stars left (next iteration limit 5397)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits N_match=4906 sigma_overall_arcsec=0.330 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.447 sigma_q3_arcsec=0.286 sigma_q4_arcsec=0.303 n_q1=1581 n_q2=883 n_q3=1465 n_q4=977 worst_quadrant_to_overall_ratio=1.355
The image catalog is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -region wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.4SHi7bxduV (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_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.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_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
Checking if the catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
WCS catalog name: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=266, bad_region=888, passed=4916
Got 4916 stars (including 3848 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat
util/solve_plate_with_UCAC5 got 4916 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3791 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3781 matched stars entering correct_measured_positions(), 3781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3781 matched stars entering correct_measured_positions(), 4239 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3790 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3782 matched stars entering correct_measured_positions(), 4239 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 3782 matched stars entering correct_measured_positions(), 4239 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 3782 stars left (next iteration limit 4159)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3782 robust_rms=6.246 arcsec worst_quadrant_rms=7.683 arcsec
SIP_REFIT: SIP order 3 trial: matched=3782 robust_rms=0.542 arcsec worst_quadrant_rms=0.578 arcsec
SIP_REFIT: SIP order 5 trial: matched=3782 robust_rms=0.500 arcsec worst_quadrant_rms=0.533 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3782 robust_rms_before=0.921 arcsec robust_rms_before_corrected=0.462 arcsec robust_rms_after=0.500 arcsec worst_quadrant_rms_before=0.511 worst_quadrant_rms_after=0.533
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.511 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits N_match=3782 sigma_overall_arcsec=0.468 sigma_q1_arcsec=0.433 sigma_q2_arcsec=0.532 sigma_q3_arcsec=0.464 sigma_q4_arcsec=0.491 n_q1=1323 n_q2=701 n_q3=1090 n_q4=668 worst_quadrant_to_overall_ratio=1.138
The image catalog is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits -region wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.3tu4ZNh1mt (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_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.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_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
Checking if the catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
WCS catalog name: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=237, bad_region=868, passed=4900
Got 4900 stars (including 3863 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat
util/solve_plate_with_UCAC5 got 4900 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 3803 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3794 matched stars entering correct_measured_positions(), 3794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3794 matched stars entering correct_measured_positions(), 4242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 3803 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3795 matched stars entering correct_measured_positions(), 4242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 3795 matched stars entering correct_measured_positions(), 4242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 3795 stars left (next iteration limit 4173)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3795 robust_rms=6.250 arcsec worst_quadrant_rms=8.343 arcsec
SIP_REFIT: SIP order 3 trial: matched=3795 robust_rms=0.522 arcsec worst_quadrant_rms=0.528 arcsec
SIP_REFIT: SIP order 5 trial: matched=3795 robust_rms=0.478 arcsec worst_quadrant_rms=0.507 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=3795 robust_rms_before=0.941 arcsec robust_rms_before_corrected=0.452 arcsec robust_rms_after=0.522 arcsec worst_quadrant_rms_before=0.487 worst_quadrant_rms_after=0.528
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.487 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits N_match=3795 sigma_overall_arcsec=0.455 sigma_q1_arcsec=0.433 sigma_q2_arcsec=0.488 sigma_q3_arcsec=0.467 sigma_q4_arcsec=0.453 n_q1=1336 n_q2=687 n_q3=1095 n_q4=677 worst_quadrant_to_overall_ratio=1.072
The image catalog is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits -region wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits to local_wcs_cache/
'wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits' -> 'local_wcs_cache/wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits'
Saving the final (post-refit) wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits to local_wcs_cache/
'wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits' -> 'local_wcs_cache/wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits'
Saving the final (post-refit) wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits'
Saving the final (post-refit) wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits sigma_overall=0.327 worst_q_ratio=1.338
ref2=Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits sigma_overall=0.330 worst_q_ratio=1.355
new1=fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits sigma_overall=0.468 worst_q_ratio=1.138
new2=fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits sigma_overall=0.455 worst_q_ratio=1.072
reference average sigma_overall=0.3285 worst_q_ratio=1.3465
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_astrometric_residuals.png (4906 matched stars from wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_astrometric_residuals.png (4906 matched stars from wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126_astrometric_residuals.png (3782 matched stars from wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127_astrometric_residuals.png (3795 matched stars from wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits'
Saving fully-calibrated image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits'
Preparing the HTML report for the field Sco-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:13:59.46 -08:07:31.4: 11.92 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:26:54.98 -09:51:38.8: 12.06 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:26:54.98 -09:51:38.8: 12.07 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:13:59.46 -08:07:31.4: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Forced photometry filter REJECTED candidate at 16:26:54.98 -09:51:38.8: ref_mag=12.07 +/- 0.01 new_mean_mag=11.9106 delta=0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:13:59.46 -08:07:31.4: ref_mag=11.91 +/- 0.01 new_mean_mag=11.8379 delta=0.08 (need > 0.90)
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 20476_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 20476_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 15:59:10.72 -14:10:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20499_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 20499_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:23:15.78 -13:57:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20520_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 20520_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:26:54.20 -09:46:05.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20529_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 20529_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20534_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 20534_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02078_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 02078_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:21:24.40 -07:42:02.5 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-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
SExtractor catalog cache: saved Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Creating symlink local_wcs_cache/wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
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-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits exists and is non-empty
wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits exists and is non-empty
wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits exists and is non-empty
wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (1st reference image)
verification OK: wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:07.919 -09:59:23.60 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits (1st new image)
verification OK: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:17:07.915 -10:00:04.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:07.919 -09:59:23.60
Second-epoch image center 16:17:07.915 -10:00:04.22
Angular distance between the image centers 0.0113 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits (2nd new image)
verification OK: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 16:17:06.452 -09:59:31.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:17:07.919 -09:59:23.60
Second-epoch image center 16:17:06.452 -09:59:31.35
Angular distance between the image centers 0.0064 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 16:17:07.915 -10:00:04.22
Second-epoch second image center 16:17:06.452 -09:59:31.35
Angular distance between the image centers 0.01093 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-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits &> /tmp/tmp.dEEVQOBOi0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits &> /tmp/tmp.dEv2Cx6zAK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits &> /tmp/tmp.GikFQwEeQy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits &> /tmp/tmp.0bresUxxZT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
Found non-empty wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
The reference image (wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits) and catalog (wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat) found
'wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat' -> 'wcsmag.cat'
Read 66506 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 deg
Loaded 5306 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3762 out of 4283 total matches.
Matched with Tycho-2 4283 out of 66506 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.684850
a=0.000000 b=1.000000 c=22.684850
From vast_summary.log: estimated ref. image limiting mag.: -7.37
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 66506 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 deg
Loaded 5306 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3762 out of 4283 total matches.
Matched with Tycho-2 4283 out of 66506 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -> calib.txt_param_ref_wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (aperture=4.4)
Read 66556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8740 to 252.4990 deg, Dec -15.6083 to -4.1791 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8740 to 252.4990 deg, Dec -15.6083 to -4.1791 deg
Loaded 5298 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3780 out of 4279 total matches.
Matched with Tycho-2 4279 out of 66556 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -> calib.txt_param_ref_wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 28 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
1.9 pix Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
2.3 pix fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
2.4 pix fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
Limiting magnitude estimates:
15.3 mag. Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
15.3 mag. Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
14.5 mag. fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
14.4 mag. fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 14.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dEEVQOBOi0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits' -> 'wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS-calibrated image found: wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Checking if the catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS catalog name: wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=3301, bad_region=11966, passed=66491
Got 66491 stars (including 51695 good ones) from the SExtractor catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 66491 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 4922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 57292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4921 matched stars entering correct_measured_positions(), 57292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4921 matched stars entering correct_measured_positions(), 57292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4921 stars left (next iteration limit 5414)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits N_match=4921 sigma_overall_arcsec=0.326 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.414 sigma_q3_arcsec=0.285 sigma_q4_arcsec=0.306 n_q1=1605 n_q2=894 n_q3=1466 n_q4=956 worst_quadrant_to_overall_ratio=1.270
The image catalog is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -region wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.dEv2Cx6zAK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits' -> 'wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS-calibrated image found: wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Checking if the catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS catalog name: wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=21, blended=3301, bad_region=11919, passed=66535
Got 66535 stars (including 51766 good ones) from the SExtractor catalog wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat
util/solve_plate_with_UCAC5 got 66535 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4921 matched stars entering correct_measured_positions(), 4921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4921 matched stars entering correct_measured_positions(), 57416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 57416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 57416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4920 stars left (next iteration limit 5413)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits N_match=4920 sigma_overall_arcsec=0.326 sigma_q1_arcsec=0.328 sigma_q2_arcsec=0.422 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.304 n_q1=1607 n_q2=888 n_q3=1474 n_q4=951 worst_quadrant_to_overall_ratio=1.298
The image catalog is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -region wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.GikFQwEeQy (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_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.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_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
Checking if the catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
WCS catalog name: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=1744, bad_region=3946, passed=35316
Got 35316 stars (including 30255 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat
util/solve_plate_with_UCAC5 got 35316 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 4899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 32391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 32391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 32391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4900 stars left (next iteration limit 5388)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4900 robust_rms=5.853 arcsec worst_quadrant_rms=9.938 arcsec
SIP_REFIT: SIP order 3 trial: matched=4900 robust_rms=0.550 arcsec worst_quadrant_rms=0.584 arcsec
SIP_REFIT: SIP order 5 trial: matched=4900 robust_rms=0.507 arcsec worst_quadrant_rms=0.540 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4900 robust_rms_before=0.941 arcsec robust_rms_before_corrected=0.469 arcsec robust_rms_after=0.507 arcsec worst_quadrant_rms_before=0.515 worst_quadrant_rms_after=0.540
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.515 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits N_match=4900 sigma_overall_arcsec=0.474 sigma_q1_arcsec=0.451 sigma_q2_arcsec=0.511 sigma_q3_arcsec=0.469 sigma_q4_arcsec=0.493 n_q1=1735 n_q2=807 n_q3=1544 n_q4=814 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits -region wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.0bresUxxZT (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_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.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_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
Checking if the catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
WCS catalog name: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=1, blended=1705, bad_region=3840, passed=34413
Got 34413 stars (including 29431 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat
util/solve_plate_with_UCAC5 got 34413 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 4902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4902 matched stars entering correct_measured_positions(), 31563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 31563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 31563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4901 stars left (next iteration limit 5392)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4901 robust_rms=5.914 arcsec worst_quadrant_rms=10.043 arcsec
SIP_REFIT: SIP order 3 trial: matched=4901 robust_rms=0.541 arcsec worst_quadrant_rms=0.548 arcsec
SIP_REFIT: SIP order 5 trial: matched=4901 robust_rms=0.492 arcsec worst_quadrant_rms=0.518 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4901 robust_rms_before=0.960 arcsec robust_rms_before_corrected=0.461 arcsec robust_rms_after=0.492 arcsec worst_quadrant_rms_before=0.489 worst_quadrant_rms_after=0.518
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.489 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits N_match=4901 sigma_overall_arcsec=0.468 sigma_q1_arcsec=0.459 sigma_q2_arcsec=0.502 sigma_q3_arcsec=0.474 sigma_q4_arcsec=0.465 n_q1=1744 n_q2=802 n_q3=1532 n_q4=823 worst_quadrant_to_overall_ratio=1.071
The image catalog is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits -region wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.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_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-37-50_20.00sec_-0.00C_LIGHT_0126.fits
Saving fully-calibrated image wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.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_2026-09-07_CI_Sco-01-Q2b1x1_224751_TTUQ2b1x1_3090758_78KAAaCr/wcs_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127.fits
Preparing the HTML report for the field Sco-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:27:08.78 -13:07:29.8: 11.85 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:31:14.90 -13:45:44.5: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:36:08.54 -11:27:28.0: 13.97 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:29:25.90 -13:32:43.2: 13.05 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:44:41.83 -12:37:18.8: 13.48 +/- 0.05 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:33:16.71 -12:48:20.4: 13.40 +/- 0.05 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:29:25.90 -13:32:43.2: 13.11 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:27:08.78 -13:07:29.8: 11.79 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:44:41.83 -12:37:18.8: 13.24 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:31:14.90 -13:45:44.5: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:36:08.54 -11:27:28.0: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter REJECTED candidate at 16:29:25.90 -13:32:43.2: ref_mag=13.08 +/- 0.03 new_mean_mag=12.9884 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Forced photometry reference-image weighted average: 13.34 +/- 0.03
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Forced photometry filter REJECTED candidate at 16:27:08.78 -13:07:29.8: ref_mag=11.82 +/- 0.01 new_mean_mag=11.9197 delta=-0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:44:41.83 -12:37:18.8: ref_mag=13.34 +/- 0.03 new_mean_mag=13.3771 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:36:08.54 -11:27:28.0: ref_mag=13.98 +/- 0.05 new_mean_mag=13.8601 delta=0.12 (need > 0.90)
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:32:27.23 -12:45:57.4: 13.82 +/- 0.06 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:26:14.14 -07:19:33.5: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:33:16.71 -12:48:20.4: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry filter REJECTED candidate at 16:33:16.71 -12:48:20.4: ref_mag=13.42 +/- 0.03 new_mean_mag=13.2736 delta=0.14 (need > 0.90)
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:32:27.23 -12:45:57.4: 13.73 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Forced photometry filter REJECTED candidate at 16:32:27.23 -12:45:57.4: ref_mag=13.77 +/- 0.04 new_mean_mag=13.7076 delta=0.06 (need > 0.90)
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:26:14.14 -07:19:33.5: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:13:37.92 -06:02:02.3: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:38:14.30 -11:20:29.0: 15.01 +/- 0.18 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:18:28.01 -08:11:45.1: 13.20 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:13:37.92 -06:02:02.3: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:38:14.30 -11:20:29.0: 14.84 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.11
Forced photometry filter REJECTED candidate at 16:38:14.30 -11:20:29.0: ref_mag=14.91 +/- 0.11 new_mean_mag=14.1240 delta=0.79 (need > 0.90)
Forced photometry on wcs_Sco-01-Q2b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:18:28.01 -08:11:45.1: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 16:18:28.01 -08:11:45.1: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2668 delta=0.96 (need > 0.90)
Adding exclusion_list_local.txt__out22274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82317.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: 5s
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Considering the candidate 81560_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81560_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
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Considering the candidate 81565_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81565_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
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Considering the candidate 81571_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81571_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:31:46.35 -12:26:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81576_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81576_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81660_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81660_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:23:15.78 -13:57:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81736_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81736_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:38:16.52 -07:06:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81814_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
Preparing report for the candidate 81814_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
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Considering the candidate 81831_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81831_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:22:34.09 -12:26:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81895_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81895_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:02:58.18 -05:49:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81919_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81919_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
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Considering the candidate 81923_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81923_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:37:29.51 -11:51:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81925_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81925_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:07:19.81 -13:09:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81932_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81932_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
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Considering the candidate 81940_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81940_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:19:02.85 -07:20:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81984_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 81984_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:17:42.73 -06:07:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82097_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 82097_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:27:41.66 -08:21:18.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82113_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 82113_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
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Considering the candidate 82131_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
Preparing report for the candidate 82131_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
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Considering the candidate 82166_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 82166_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:11:52.17 -10:03:55.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82229_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 82229_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:26:26.30 -06:56:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82258_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 82258_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:15:44.75 -08:22:31.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82280_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 82280_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
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Considering the candidate 82317_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
Preparing report for the candidate 82317_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
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Considering the candidate 17754_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 17754_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:21:24.40 -07:42:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11419_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 11419_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:13:53.53 -06:32:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12604_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 12604_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks
**** FOUND 16:07:45.59 -06:37:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22274_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
Preparing report for the candidate 22274_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
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Considering the candidate 32325_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127
The candidate 32325_fd_Sco-01-Q2b1x1_2026-09-07_22-38-37_20.00sec_-0.00C_LIGHT_0127 did not pass the final checks