This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 04.1841 2461256.6841 12.40 16:11:34.45 -10:47:04.9
1.82737 28.44061 galactic Sco Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.28 Bellona 0 -0 0 12.6 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:11:34.45 -10:47:04.9: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:11:34.45 -10:47:04.9: 15.95 +/- 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,2461256.6841,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260804.1841 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 04.1841 2461256.6841 12.69 16:29:30.74 -05:11:39.7
9.93633 28.24090 galactic Oph Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.258 Tyche 1 -0 1 12.8 0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:29:30.74 -05:11:39.7: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:29:30.74 -05:11:39.7: 15.83 +/- 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,2461256.6841,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260804.1841 12.69CV 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 08 04.1841 2461256.6841 12.80 16:18:20.45 -13:36:37.0
0.54662 25.37247 galactic Sco Second-epoch detections are separated by 0.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.48 Doris 1 0 1 12.8 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:18:20.45 -13:36:37.0: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:18:20.45 -13:36:37.0: 15.90 +/- 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,2461256.6841,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260804.1841 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 04.1841 2461256.6841 13.18 16:27:27.90 -14:51:30.5
1.00733 22.86857 galactic Oph Second-epoch detections are separated by 1.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.119 Althaea 1 0 1 13.0 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:27:27.90 -14:51:30.5: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:27:27.90 -14:51:30.5: 15.68 +/- 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,2461256.6841,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260804.1841 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 04.1841 2461256.6841 13.62 15:55:54.40 -06:36:57.2
2.74291 34.07542 galactic Lib Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.97 Klotho 1 -1 1 13.6 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:55:54.40 -06:36:57.2: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:55:54.40 -06:36:57.2: 15.89 +/- 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,2461256.6841,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260804.1841 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 04.1841 2461256.6841 14.32 15:52:12.15 -10:28:10.6
358.53002 32.27021 galactic Lib Second-epoch detections are separated by 2.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.323 Brucia -1 -0 1 14.4 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:52:12.15 -10:28:10.6: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:52:12.15 -10:28:10.6: 15.83 +/- 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,2461256.6841,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260804.1841 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461174.84044517 14.05.2026 08:10:04.463 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
First image: 2461174.84044517 14.05.2026 08:10:04.463 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Last image: 2461256.68443860 04.08.2026 04:25:25.495 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 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): 7770
Objects passed selection criteria: 7766
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 7150.75
Average stars matched: 7017.5 (98.1366 %)
Memory usage VmPeak: 234060 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 3 23:36:58 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461174.84044517 14.05.2026 08:10:04.463 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
First image: 2461174.84044517 14.05.2026 08:10:04.463 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Last image: 2461256.68443860 04.08.2026 04:25:25.495 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 52
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 65 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): 61594
Objects passed selection criteria: 61478
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 57207.5
Average stars matched: 55544 (97.0922 %)
Memory usage VmPeak: 282132 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 3 23:39:16 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.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: 2461256.68367222
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits exists and is non-empty
Saving wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits to local_wcs_cache/
'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits' -> 'local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits'
wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits exists and is non-empty
Saving wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits to local_wcs_cache/
'wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits' -> 'local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits'
wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits exists and is non-empty
Saving wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits'
wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits exists and is non-empty
Saving wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (1st reference image)
verification OK: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:07.919 -09:59:23.60 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits (1st new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
Image size: 941.1'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:06.287 -09:57:46.39 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 16:17:06.287 -09:57:46.39
Angular distance between the image centers 0.0278 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits (2nd new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Image size: 941.1'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:04.452 -09:57:13.87 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 16:17:04.452 -09:57:13.87
Angular distance between the image centers 0.0387 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 16:17:06.287 -09:57:46.39
Second-epoch second image center 16:17:04.452 -09:57:13.87
Angular distance between the image centers 0.01176 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits &> /tmp/tmp.TO8adWdEUg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits &> /tmp/tmp.mENt2iuqmr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits &> /tmp/tmp.6m0ceA7rG0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits &> /tmp/tmp.3SnxfZcAhD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
The reference image (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits) and catalog (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat) found
'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat' -> 'wcsmag.cat'
Read 8279 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 deg
Loaded 5209 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4038 out of 4209 total matches.
Matched with Tycho-2 4209 out of 8279 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.855250
a=0.000000 b=1.000000 c=22.855250
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8279 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8992 to 252.4575 deg, Dec -15.6003 to -4.3252 deg
Loaded 5209 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4038 out of 4209 total matches.
Matched with Tycho-2 4209 out of 8279 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (aperture=6.2)
Read 8296 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8990 to 252.4990 deg, Dec -15.6005 to -4.3251 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8990 to 252.4990 deg, Dec -15.6005 to -4.3251 deg
Loaded 5223 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4035 out of 4212 total matches.
Matched with Tycho-2 4212 out of 8296 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
2.2 pix Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
2.3 pix fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
2.3 pix fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Limiting magnitude estimates:
15.1 mag. Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
15.1 mag. Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
14.7 mag. fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
14.7 mag. fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.TO8adWdEUg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=513, bad_region=0, passed=8279
Got 8279 stars (including 7758 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 8279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 8279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 8279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 8279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4907 stars left (next iteration limit 5397)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits N_match=4907 sigma_overall_arcsec=0.319 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.368 sigma_q3_arcsec=0.271 sigma_q4_arcsec=0.292 n_q1=1253 n_q2=1184 n_q3=1109 n_q4=1361 worst_quadrant_to_overall_ratio=1.156
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.mENt2iuqmr (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=538, bad_region=0, passed=8296
Got 8296 stars (including 7747 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat
util/solve_plate_with_UCAC5 got 8296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4912 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits N_match=4912 sigma_overall_arcsec=0.319 sigma_q1_arcsec=0.351 sigma_q2_arcsec=0.354 sigma_q3_arcsec=0.257 sigma_q4_arcsec=0.295 n_q1=1257 n_q2=1189 n_q3=1108 n_q4=1358 worst_quadrant_to_overall_ratio=1.112
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6m0ceA7rG0 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=303, bad_region=0, passed=6133
Got 6133 stars (including 5825 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat
util/solve_plate_with_UCAC5 got 6133 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 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: 4904 matched stars entering correct_measured_positions(), 4904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 6133 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 372 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: 4904 matched stars entering correct_measured_positions(), 6133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 6133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4904 stars left (next iteration limit 5394)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4904 robust_rms=9.761 arcsec worst_quadrant_rms=10.791 arcsec
SIP_REFIT: SIP order 3 trial: matched=4904 robust_rms=0.412 arcsec worst_quadrant_rms=0.421 arcsec
SIP_REFIT: SIP order 5 trial: matched=4904 robust_rms=0.292 arcsec worst_quadrant_rms=0.303 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4904 robust_rms_before=0.810 arcsec robust_rms_before_corrected=0.299 arcsec robust_rms_after=0.292 arcsec worst_quadrant_rms_before=0.331 worst_quadrant_rms_after=0.303
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.331 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits N_match=4904 sigma_overall_arcsec=0.311 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.329 sigma_q3_arcsec=0.278 sigma_q4_arcsec=0.290 n_q1=1264 n_q2=1189 n_q3=1121 n_q4=1330 worst_quadrant_to_overall_ratio=1.103
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits -region wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3SnxfZcAhD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=309, bad_region=0, passed=6111
Got 6111 stars (including 5795 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat
util/solve_plate_with_UCAC5 got 6111 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.5 to -4.3)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 4910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 6111 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 372 to 430 (Dec -15.5 to -4.3)
Done reading UCAC5 zone files...
Matched 4923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 6111 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 6111 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4909 stars left (next iteration limit 5399)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4909 robust_rms=9.726 arcsec worst_quadrant_rms=10.730 arcsec
SIP_REFIT: SIP order 3 trial: matched=4909 robust_rms=0.392 arcsec worst_quadrant_rms=0.397 arcsec
SIP_REFIT: SIP order 5 trial: matched=4909 robust_rms=0.301 arcsec worst_quadrant_rms=0.312 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4909 robust_rms_before=0.797 arcsec robust_rms_before_corrected=0.308 arcsec robust_rms_after=0.301 arcsec worst_quadrant_rms_before=0.331 worst_quadrant_rms_after=0.312
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.331 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits N_match=4909 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.347 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.291 sigma_q4_arcsec=0.309 n_q1=1267 n_q2=1183 n_q3=1120 n_q4=1339 worst_quadrant_to_overall_ratio=1.100
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits -region wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits sigma_overall=0.319 worst_q_ratio=1.156
ref2=Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits sigma_overall=0.319 worst_q_ratio=1.112
new1=fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits sigma_overall=0.311 worst_q_ratio=1.103
new2=fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits sigma_overall=0.315 worst_q_ratio=1.100
reference average sigma_overall=0.319 worst_q_ratio=1.134
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162_astrometric_residuals.png (4907 matched stars from wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163_astrometric_residuals.png (4912 matched stars from wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118_astrometric_residuals.png (4904 matched stars from wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119_astrometric_residuals.png (4909 matched stars from wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits'
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits'
Preparing the HTML report for the field Sco-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:13:59.45 -08:07:31.6: 11.92 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:26:54.96 -09:51:38.6: 12.06 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:59:10.72 -14:10:55.7: 12.81 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:59:10.72 -14:10:55.7: 12.81 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:13:59.45 -08:07:31.6: 11.91 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:26:54.96 -09:51:38.6: 12.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter REJECTED candidate at 15:59:10.72 -14:10:55.7: ref_mag=12.81 +/- 0.02 new_mean_mag=12.1596 delta=0.65 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:13:59.45 -08:07:31.6: ref_mag=11.92 +/- 0.01 new_mean_mag=11.8929 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:26:54.96 -09:51:38.6: ref_mag=12.07 +/- 0.01 new_mean_mag=12.0223 delta=0.04 (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 20512_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 20512_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:44:41.84 -14:41:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20515_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 20515_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:26:54.26 -09:46:05.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20516_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 20516_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20518_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 20518_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20521_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 20521_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02078_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 02078_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:21:24.46 -07:42:01.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02024_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 02024_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:45:23.15 -07:56:25.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Sco-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Creating symlink local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits exists and is non-empty
wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits exists and is non-empty
wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits exists and is non-empty
wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (1st reference image)
verification OK: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:07.919 -09:59:23.60 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits (1st new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
Image size: 941.1'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:06.287 -09:57:46.39 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 16:17:06.287 -09:57:46.39
Angular distance between the image centers 0.0278 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits (2nd new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Image size: 941.1'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:04.452 -09:57:13.87 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 16:17:04.452 -09:57:13.87
Angular distance between the image centers 0.0387 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 16:17:06.287 -09:57:46.39
Second-epoch second image center 16:17:04.452 -09:57:13.87
Angular distance between the image centers 0.01176 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits &> /tmp/tmp.j9SWrrJNiA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits &> /tmp/tmp.nCLLEBGiWJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits &> /tmp/tmp.vOm5OxEByt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits &> /tmp/tmp.Y7Mdrbx8Gf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
Found non-empty wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits and wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
The reference image (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits) and catalog (wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat) found
'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat' -> 'wcsmag.cat'
Read 66506 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 deg
Loaded 5306 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3762 out of 4283 total matches.
Matched with Tycho-2 4283 out of 66506 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.698250
a=0.000000 b=1.000000 c=22.698250
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 66506 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8513 to 252.4891 deg, Dec -15.6160 to -4.1921 deg
Loaded 5306 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3762 out of 4283 total matches.
Matched with Tycho-2 4283 out of 66506 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits (aperture=4.5)
Read 66556 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.8740 to 252.4990 deg, Dec -15.6083 to -4.1791 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 235.8740 to 252.4990 deg, Dec -15.6083 to -4.1791 deg
Loaded 5298 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3780 out of 4279 total matches.
Matched with Tycho-2 4279 out of 66556 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 47 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
1.9 pix Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
2.2 pix fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
2.2 pix fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Limiting magnitude estimates:
15.3 mag. Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
15.3 mag. Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
14.9 mag. fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
14.8 mag. fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.3 (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.j9SWrrJNiA (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=3301, bad_region=1, passed=66487
Got 66487 stars (including 63074 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 66487 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 4918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 66487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 66487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 66487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4918 stars left (next iteration limit 5409)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits N_match=4918 sigma_overall_arcsec=0.309 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.345 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.285 n_q1=1250 n_q2=1191 n_q3=1117 n_q4=1360 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nCLLEBGiWJ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits' -> 'wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat corresponding to the image wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=3301, bad_region=1, passed=66529
Got 66529 stars (including 63096 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat
util/solve_plate_with_UCAC5 got 66529 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 4922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 66529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4921 matched stars entering correct_measured_positions(), 66529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4921 matched stars entering correct_measured_positions(), 66529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4921 stars left (next iteration limit 5414)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits N_match=4921 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.343 sigma_q3_arcsec=0.259 sigma_q4_arcsec=0.290 n_q1=1255 n_q2=1190 n_q3=1119 n_q4=1357 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits -region wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.vOm5OxEByt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1724, bad_region=4, passed=48557
Got 48557 stars (including 46764 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat
util/solve_plate_with_UCAC5 got 48557 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 4911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 48557 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 372 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 48557 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 48557 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4912 stars left (next iteration limit 5402)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits N_match=4912 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.323 sigma_q3_arcsec=0.275 sigma_q4_arcsec=0.282 n_q1=1267 n_q2=1195 n_q3=1118 n_q4=1332 worst_quadrant_to_overall_ratio=1.073
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits -region wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Y7Mdrbx8Gf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1741, bad_region=5, passed=48710
Got 48710 stars (including 46896 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat
util/solve_plate_with_UCAC5 got 48710 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 48710 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 372 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 4923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 48710 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 48710 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4913 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits N_match=4913 sigma_overall_arcsec=0.309 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.307 sigma_q3_arcsec=0.291 sigma_q4_arcsec=0.294 n_q1=1262 n_q2=1186 n_q3=1120 n_q4=1345 worst_quadrant_to_overall_ratio=1.066
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits -region wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-24-19_20.00sec_-0.00C_LIGHTs_0118.fits
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Sco-01-Q1b1x1_233108_TTUQ1b1x1_732136_aJxWccyU/wcs_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119.fits
Preparing the HTML report for the field Sco-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:27:08.78 -13:07:29.8: 11.84 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:31:48.89 -08:00:30.2: 14.23 +/- 0.08 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:33:24.90 -15:02:05.9: 13.27 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:13:02.51 -07:24:31.1: 14.73 +/- 0.11 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:11:32.94 -11:14:53.8: 14.12 +/- 0.08 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:06:54.88 -07:42:02.3: 11.90 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:11:34.45 -10:47:04.9: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:13:02.51 -07:24:31.1: 14.83 +/- 0.12 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:06:54.88 -07:42:02.3: 11.90 +/- 0.01 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:11:32.94 -11:14:53.8: 14.22 +/- 0.08 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:33:24.90 -15:02:05.9: 13.18 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:31:48.89 -08:00:30.2: 14.22 +/- 0.08 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:27:08.78 -13:07:29.8: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 14.16 +/- 0.06
Forced photometry reference-image weighted average: 14.77 +/- 0.08
Forced photometry filter REJECTED candidate at 16:11:32.94 -11:14:53.8: ref_mag=14.16 +/- 0.06 new_mean_mag=14.2519 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 14.23 +/- 0.06
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Forced photometry filter REJECTED candidate at 16:13:02.51 -07:24:31.1: ref_mag=14.77 +/- 0.08 new_mean_mag=14.6007 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Forced photometry filter REJECTED candidate at 16:06:54.88 -07:42:02.3: ref_mag=11.90 +/- 0.01 new_mean_mag=12.1190 delta=-0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:31:48.89 -08:00:30.2: ref_mag=14.23 +/- 0.06 new_mean_mag=14.2853 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:33:24.90 -15:02:05.9: ref_mag=13.22 +/- 0.03 new_mean_mag=13.3510 delta=-0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:27:08.78 -13:07:29.8: ref_mag=11.80 +/- 0.01 new_mean_mag=12.0571 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:29:30.74 -05:11:39.7: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:11:34.45 -10:47:04.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:29:30.74 -05:11:39.7: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:18:20.45 -13:36:37.0: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:19:59.24 -14:38:20.3: 13.39 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:19:02.77 -07:20:01.2: 13.28 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:47:36.40 -14:00:46.3: 13.37 +/- 0.05 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:27:27.90 -14:51:30.5: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:18:20.45 -13:36:37.0: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:22:34.16 -12:26:11.1: 12.82 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:21:52.00 -07:08:17.0: 13.66 +/- 0.05 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:19:59.24 -14:38:20.3: 13.36 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:19:02.77 -07:20:01.2: 13.33 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 16:19:59.24 -14:38:20.3: ref_mag=13.38 +/- 0.03 new_mean_mag=13.4431 delta=-0.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter REJECTED candidate at 16:19:02.77 -07:20:01.2: ref_mag=13.30 +/- 0.03 new_mean_mag=13.3133 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:27:27.90 -14:51:30.5: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:47:36.40 -14:00:46.3: 13.30 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.03
Forced photometry filter REJECTED candidate at 15:47:36.40 -14:00:46.3: ref_mag=13.33 +/- 0.03 new_mean_mag=13.4901 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:22:34.16 -12:26:11.1: 12.81 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:55:54.40 -06:36:57.2: 15.92 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter REJECTED candidate at 16:22:34.16 -12:26:11.1: ref_mag=12.81 +/- 0.02 new_mean_mag=12.8586 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:21:52.00 -07:08:17.0: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Forced photometry filter REJECTED candidate at 16:21:52.00 -07:08:17.0: ref_mag=13.64 +/- 0.03 new_mean_mag=13.6322 delta=0.01 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:55:54.40 -06:36:57.2: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:45:31.43 -10:54:58.3: 13.65 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:32:05.40 -12:08:24.0: 13.95 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:59:52.64 -07:02:50.2: 13.83 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:45:31.43 -10:54:58.3: 13.67 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.05
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:26:39.04 -08:42:28.9: 13.94 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 16:45:31.43 -10:54:58.3: ref_mag=13.66 +/- 0.05 new_mean_mag=13.5710 delta=0.09 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:13:17.59 -10:21:36.6: 14.02 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:32:05.40 -12:08:24.0: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Forced photometry filter REJECTED candidate at 16:32:05.40 -12:08:24.0: ref_mag=13.90 +/- 0.05 new_mean_mag=13.8028 delta=0.10 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:59:52.64 -07:02:50.2: 13.78 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.05
Forced photometry filter REJECTED candidate at 15:59:52.64 -07:02:50.2: ref_mag=13.81 +/- 0.05 new_mean_mag=13.8583 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:26:39.04 -08:42:28.9: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter REJECTED candidate at 16:26:39.04 -08:42:28.9: ref_mag=13.93 +/- 0.04 new_mean_mag=13.9103 delta=0.01 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:13:17.59 -10:21:36.6: 13.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Forced photometry filter REJECTED candidate at 16:13:17.59 -10:21:36.6: ref_mag=13.98 +/- 0.05 new_mean_mag=14.0009 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:09:16.25 -11:32:06.7: 14.28 +/- 0.09 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:26:48.57 -09:50:40.5: 13.74 +/- 0.08 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 15:52:12.15 -10:28:10.6: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:09:16.25 -11:32:06.7: 14.07 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Forced photometry filter REJECTED candidate at 16:09:16.25 -11:32:06.7: ref_mag=14.17 +/- 0.06 new_mean_mag=14.2078 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:32:24.94 -11:08:24.0: 14.56 +/- 0.13 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 15:52:12.15 -10:28:10.6: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:32:24.94 -11:08:24.0: 14.85 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.10
Forced photometry filter REJECTED candidate at 16:32:24.94 -11:08:24.0: ref_mag=14.68 +/- 0.10 new_mean_mag=14.4677 delta=0.21 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:26:48.57 -09:50:40.5: 13.83 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.06
Forced photometry filter REJECTED candidate at 16:26:48.57 -09:50:40.5: ref_mag=13.78 +/- 0.06 new_mean_mag=14.3336 delta=-0.55 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:14:08.72 -07:32:01.1: 14.39 +/- 0.08 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:05:14.72 -13:35:15.0: 15.25 +/- 0.20 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:14:08.72 -07:32:01.1: 14.37 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.06
Forced photometry filter REJECTED candidate at 16:14:08.72 -07:32:01.1: ref_mag=14.38 +/- 0.06 new_mean_mag=14.5383 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:18:00.12 -11:44:59.3: 14.61 +/- 0.13 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:05:14.72 -13:35:15.0: 14.97 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.13
Forced photometry filter REJECTED candidate at 16:05:14.72 -13:35:15.0: ref_mag=15.08 +/- 0.13 new_mean_mag=14.5891 delta=0.49 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-10-04_20.00sec_-4.90C_LIGHTs_0162.fits at 16:28:49.09 -10:47:28.6: 15.30 +/- 0.22 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:18:00.12 -11:44:59.3: 14.93 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.73 +/- 0.10
Forced photometry filter REJECTED candidate at 16:18:00.12 -11:44:59.3: ref_mag=14.73 +/- 0.10 new_mean_mag=14.8482 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-05-14_03-11-00_20.00sec_-4.90C_LIGHTs_0163.fits at 16:28:49.09 -10:47:28.6: 15.22 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.15
Forced photometry filter REJECTED candidate at 16:28:49.09 -10:47:28.6: ref_mag=15.26 +/- 0.15 new_mean_mag=14.7308 delta=0.53 (need > 0.90)
Adding exclusion_list_local.txt__out82537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82685.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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 82489_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82489_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82496_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82496_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82498_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82498_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82508_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82508_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:44:26.35 -09:44:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82509_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82509_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:47:18.04 -06:32:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82511_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82511_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82512_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82512_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:46:18.62 -07:12:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82514_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82514_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:32:12.66 -15:05:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82517_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82517_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82518_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82518_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82537_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 82537_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 82540_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82540_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:46:30.61 -12:31:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82545_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 82545_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 82548_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82548_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:39:20.32 -08:32:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82549_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 82549_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 82550_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82550_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:02:58.17 -05:49:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82553_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82553_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82571_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 82571_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 82587_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82587_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82597_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82597_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:33:16.65 -12:48:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82598_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82598_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82600_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82600_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82611_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82611_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 15:51:51.04 -11:08:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82613_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82613_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82616_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 82616_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 82618_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82618_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:11:52.10 -10:03:55.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82624_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82624_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82626_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82626_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:46:13.94 -06:26:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82630_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82630_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82639_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82639_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82642_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82642_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82651_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82651_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82676_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82676_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82683_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82683_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82685_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
Preparing report for the candidate 82685_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
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Considering the candidate 82693_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82693_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:38:16.69 -07:06:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82720_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82720_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82724_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82724_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82748_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82748_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82778_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82778_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 82779_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 82779_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
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Considering the candidate 32325_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 32325_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:26:54.25 -09:46:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09726_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 09726_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:47:48.78 -06:46:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05644_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 05644_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:28:51.18 -05:51:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48353_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 48353_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:44:41.85 -14:41:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17622_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 17622_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
**** FOUND 16:45:23.15 -07:56:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17754_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119
The candidate 17754_fd_Sco-01-Q1b1x1_2026-08-03_23-25-25_20.00sec_-0.00C_LIGHTs_0119 did not pass the final checks
