This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk
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 24.2389 2461276.7389 11.39 21:05:40.66 -08:05:24.6
41.50084 -33.45406 galactic Aqr Second-epoch detections are separated by 0.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.389 Industria -0 0 0 11.8 0 0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:05:40.66 -08:05:24.6: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:05:40.66 -08:05:24.6: 15.51 +/- 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,2461276.7389,11.39,0.05,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 20260824.2389 11.39CV 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 24.2389 2461276.7389 12.88 21:03:37.34 -12:20:39.6
36.60999 -34.86085 galactic Aqr Second-epoch detections are separated by 1.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.38 Leda 0 -0 0 13.0 -0 -0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:03:37.34 -12:20:39.6: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:03:37.34 -12:20:39.6: 15.47 +/- 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,2461276.7389,12.88,0.05,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 20260824.2389 12.88CV 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 24.2389 2461276.7389 13.54 21:36:45.98 -12:19:23.5
41.02052 -42.18637 galactic Cap Second-epoch detections are separated by 1.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.286 Iclea 0 0 0 13.5 -0 -0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:36:45.98 -12:19:23.5: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:36:45.98 -12:19:23.5: 15.52 +/- 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!
TCP 2026 08 24.2389* 21 36 45.98 -12 19 23.5 13.5 U Cap 9 0
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,2461276.7389,13.54,0.05,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 20260824.2389 13.54CV 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 24.2389 2461276.7389 13.53 21:53:54.71 -13:19:59.7
42.26579 -46.39272 galactic Cap Second-epoch detections are separated by 1.2" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2121 Sevastopol -0 -1 1 13.5 -0 -0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:53:54.71 -13:19:59.7: 15.28 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:53:54.71 -13:19:59.7: 15.19 +/- 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!
TCP 2026 08 24.2389* 21 53 54.71 -13 19 59.7 13.5 U Cap 9 0
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,2461276.7389,13.53,0.05,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 20260824.2389 13.53CV 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 24.2389 2461276.7389 13.59 21:36:18.35 -05:33:17.9
48.80514 -38.88871 galactic Aqr Second-epoch detections are separated by 1.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.685 Hermia -0 -0 0 13.3 -0 -0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:36:18.35 -05:33:17.9: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:36:18.35 -05:33:17.9: 15.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461276.7389,13.59,0.05,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 20260824.2389 13.59CV 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: 2461209.88890352 18.06.2026 09:19:51.264 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
First image: 2461209.88890352 18.06.2026 09:19:51.264 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Last image: 2461276.73915428 24.08.2026 05:44:12.930 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.84
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: 4 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): 8579
Objects passed selection criteria: 8565
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 6854.25
Average stars matched: 6619 (96.5678 %)
Memory usage VmPeak: 234692 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 24 00:52:07 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: 2461209.88890352 18.06.2026 09:19:51.264 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
First image: 2461209.88890352 18.06.2026 09:19:51.264 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Last image: 2461276.73915428 24.08.2026 05:44:12.930 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 33
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 47439
Objects passed selection criteria: 47364
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 42075.5
Average stars matched: 40435.2 (96.1017 %)
Memory usage VmPeak: 270440 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 24 00:53:23 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/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.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/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.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: 2461276.73861949
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_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits exists and is non-empty
wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits exists and is non-empty
wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits exists and is non-empty
wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (1st reference image)
verification OK: wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:43.484 -09:59:39.66 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:38.454 -09:57:42.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:43.484 -09:59:39.66
Second-epoch image center 21:25:38.454 -09:57:42.31
Angular distance between the image centers 0.0386 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:40.573 -09:57:26.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:43.484 -09:59:39.66
Second-epoch image center 21:25:40.573 -09:57:26.48
Angular distance between the image centers 0.0389 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 21:25:38.454 -09:57:42.31
Second-epoch second image center 21:25:40.573 -09:57:26.48
Angular distance between the image centers 0.00975 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/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits &> /tmp/tmp.QVIssmiXjl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits &> /tmp/tmp.PkxL6QLKKn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits &> /tmp/tmp.m7kWEKhx8p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits &> /tmp/tmp.gMipXe9Bks
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.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_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.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_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
Found non-empty wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
The reference image (wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits) and catalog (wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat) found
'wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat' -> 'wcsmag.cat'
Read 8874 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3905 to 329.4911 deg, Dec -15.2504 to -4.7005 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 313.3905 to 329.4911 deg, Dec -15.2504 to -4.7005 deg
Loaded 6721 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): 5451 out of 5615 total matches.
Matched with Tycho-2 5615 out of 8874 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.692700
a=0.000000 b=1.000000 c=22.692700
From vast_summary.log: estimated ref. image limiting mag.: -7.84
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.85
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.85
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8874 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3905 to 329.4911 deg, Dec -15.2504 to -4.7005 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 313.3905 to 329.4911 deg, Dec -15.2504 to -4.7005 deg
Loaded 6721 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): 5451 out of 5615 total matches.
Matched with Tycho-2 5615 out of 8874 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (aperture=6.4)
Read 9225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3619 to 329.4904 deg, Dec -15.2503 to -4.7004 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 313.3619 to 329.4904 deg, Dec -15.2503 to -4.7004 deg
Loaded 6736 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): 5526 out of 5688 total matches.
Matched with Tycho-2 5688 out of 9225 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
2.4 pix Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
2.5 pix fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
2.5 pix fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Limiting magnitude estimates:
14.9 mag. Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
14.9 mag. Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
14.1 mag. fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
14.1 mag. fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.QVIssmiXjl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.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/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.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=515, bad_region=0, passed=8874
Got 8874 stars (including 8351 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
util/solve_plate_with_UCAC5 got 8874 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4740 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 4713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 8874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4741 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 8874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 8874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4713 stars left (next iteration limit 5184)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits N_match=4713 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.311 sigma_q2_arcsec=0.446 sigma_q3_arcsec=0.359 sigma_q4_arcsec=0.381 n_q1=1329 n_q2=1012 n_q3=1266 n_q4=1106 worst_quadrant_to_overall_ratio=1.239
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits -region wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.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.PkxL6QLKKn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.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/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.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=511, bad_region=0, passed=9225
Got 9225 stars (including 8705 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat
util/solve_plate_with_UCAC5 got 9225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4738 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4710 matched stars entering correct_measured_positions(), 4710 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4710 matched stars entering correct_measured_positions(), 9225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4738 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4709 matched stars entering correct_measured_positions(), 9225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4709 matched stars entering correct_measured_positions(), 9225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4709 stars left (next iteration limit 5181)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits N_match=4709 sigma_overall_arcsec=0.453 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.618 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.585 n_q1=1094 n_q2=1301 n_q3=996 n_q4=1318 worst_quadrant_to_overall_ratio=1.362
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits -region wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.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.m7kWEKhx8p (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_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.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_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.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=417, bad_region=0, passed=4793
Got 4793 stars (including 4370 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 4793 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (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 -4.2)
Done reading UCAC5 zone files...
Matched 4149 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4128 matched stars entering correct_measured_positions(), 4129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4128 matched stars entering correct_measured_positions(), 4793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.5 to -4.2)
Done reading UCAC5 zone files...
Matched 4149 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4127 matched stars entering correct_measured_positions(), 4793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4127 matched stars entering correct_measured_positions(), 4793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4127 stars left (next iteration limit 4540)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4127 robust_rms=10.016 arcsec worst_quadrant_rms=16.376 arcsec
SIP_REFIT: SIP order 3 trial: matched=4127 robust_rms=0.404 arcsec worst_quadrant_rms=0.414 arcsec
SIP_REFIT: SIP order 5 trial: matched=4127 robust_rms=0.275 arcsec worst_quadrant_rms=0.305 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4127 robust_rms_before=0.917 arcsec robust_rms_before_corrected=0.292 arcsec robust_rms_after=0.275 arcsec worst_quadrant_rms_before=0.312 worst_quadrant_rms_after=0.305
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.312 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits N_match=4127 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.306 sigma_q3_arcsec=0.296 sigma_q4_arcsec=0.275 n_q1=1238 n_q2=860 n_q3=1170 n_q4=859 worst_quadrant_to_overall_ratio=1.053
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.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.gMipXe9Bks (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_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.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_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.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=371, bad_region=0, passed=4756
Got 4756 stars (including 4379 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat
util/solve_plate_with_UCAC5 got 4756 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (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 -4.2)
Done reading UCAC5 zone files...
Matched 4165 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4141 matched stars entering correct_measured_positions(), 4141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4141 matched stars entering correct_measured_positions(), 4756 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 -4.2)
Done reading UCAC5 zone files...
Matched 4166 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4141 matched stars entering correct_measured_positions(), 4756 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4141 matched stars entering correct_measured_positions(), 4756 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4141 stars left (next iteration limit 4555)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4141 robust_rms=9.818 arcsec worst_quadrant_rms=17.081 arcsec
SIP_REFIT: SIP order 3 trial: matched=4141 robust_rms=0.417 arcsec worst_quadrant_rms=0.433 arcsec
SIP_REFIT: SIP order 5 trial: matched=4141 robust_rms=0.275 arcsec worst_quadrant_rms=0.304 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4141 robust_rms_before=0.922 arcsec robust_rms_before_corrected=0.293 arcsec robust_rms_after=0.275 arcsec worst_quadrant_rms_before=0.320 worst_quadrant_rms_after=0.304
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.320 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits N_match=4141 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.322 sigma_q3_arcsec=0.289 sigma_q4_arcsec=0.278 n_q1=1260 n_q2=867 n_q3=1151 n_q4=863 worst_quadrant_to_overall_ratio=1.074
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits to local_wcs_cache/
'wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits'
Saving the final (post-refit) wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits to local_wcs_cache/
'wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits'
Saving the final (post-refit) wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits'
Saving the final (post-refit) wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits sigma_overall=0.360 worst_q_ratio=1.239
ref2=Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits sigma_overall=0.453 worst_q_ratio=1.362
new1=fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits sigma_overall=0.302 worst_q_ratio=1.053
new2=fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits sigma_overall=0.300 worst_q_ratio=1.074
reference average sigma_overall=0.4065 worst_q_ratio=1.3005
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387_astrometric_residuals.png (4713 matched stars from wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198_astrometric_residuals.png (4709 matched stars from wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212_astrometric_residuals.png (4127 matched stars from wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213_astrometric_residuals.png (4141 matched stars from wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits'
Saving fully-calibrated image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits'
Preparing the HTML report for the field Aqr-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:05:40.66 -08:05:24.6: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 20:59:16.26 -10:15:24.2: 10.48 +/- 0.00 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:05:40.66 -08:05:24.6: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 20:59:16.26 -10:15:24.2: 10.49 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.49 +/- 0.00
Forced photometry filter REJECTED candidate at 20:59:16.26 -10:15:24.2: ref_mag=10.49 +/- 0.00 new_mean_mag=10.8808 delta=-0.39 (need > 0.90)
Adding exclusion_list_local.txt__out20892.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20755_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 20755_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20892_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
Preparing report for the candidate 20892_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20022_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 20022_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
**** FOUND 21:02:32.69 -06:36:21.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Aqr-03-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 ####
21:05:40.66 -08:05:24.6
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/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Creating symlink local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits exists and is non-empty
wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits exists and is non-empty
wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits exists and is non-empty
wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (1st reference image)
verification OK: wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 21:25:43.484 -09:59:39.66 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:38.454 -09:57:42.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:43.484 -09:59:39.66
Second-epoch image center 21:25:38.454 -09:57:42.31
Angular distance between the image centers 0.0386 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Image size: 940.8'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:40.573 -09:57:26.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:43.484 -09:59:39.66
Second-epoch image center 21:25:40.573 -09:57:26.48
Angular distance between the image centers 0.0389 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 21:25:38.454 -09:57:42.31
Second-epoch second image center 21:25:40.573 -09:57:26.48
Angular distance between the image centers 0.00975 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/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits &> /tmp/tmp.HlAReSQZB5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits &> /tmp/tmp.3jl5aovn8d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits &> /tmp/tmp.C5cVVYzRAl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits &> /tmp/tmp.5mE1ZfsxBF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.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_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.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_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
Found non-empty wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits and wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
The reference image (wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits) and catalog (wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat) found
'wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat' -> 'wcsmag.cat'
Read 53069 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3814 to 329.5453 deg, Dec -15.2618 to -4.6695 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 313.3814 to 329.5453 deg, Dec -15.2618 to -4.6695 deg
Loaded 6771 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): 5405 out of 5966 total matches.
Matched with Tycho-2 5966 out of 53069 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.562200
a=0.000000 b=1.000000 c=22.562200
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.00
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.00
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 53069 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3814 to 329.5453 deg, Dec -15.2618 to -4.6695 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 313.3814 to 329.5453 deg, Dec -15.2618 to -4.6695 deg
Loaded 6771 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): 5405 out of 5966 total matches.
Matched with Tycho-2 5966 out of 53069 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (aperture=5.0)
Read 51567 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.3495 to 329.5140 deg, Dec -15.2503 to -4.6788 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 313.3495 to 329.5140 deg, Dec -15.2503 to -4.6788 deg
Loaded 6759 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): 5424 out of 5938 total matches.
Matched with Tycho-2 5938 out of 51567 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 31 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
2.3 pix Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
2.4 pix fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
2.4 pix fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Limiting magnitude estimates:
15.0 mag. Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
15.0 mag. Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
14.2 mag. fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
14.2 mag. fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.HlAReSQZB5 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.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/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.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=18, blended=2577, bad_region=1, passed=53051
Got 53051 stars (including 50399 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat
util/solve_plate_with_UCAC5 got 53051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4728 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4711 matched stars entering correct_measured_positions(), 4711 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4711 matched stars entering correct_measured_positions(), 53051 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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4728 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4710 matched stars entering correct_measured_positions(), 53051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4710 matched stars entering correct_measured_positions(), 53051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4710 stars left (next iteration limit 5182)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits N_match=4710 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.423 sigma_q3_arcsec=0.355 sigma_q4_arcsec=0.371 n_q1=1352 n_q2=1001 n_q3=1239 n_q4=1118 worst_quadrant_to_overall_ratio=1.199
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits -region wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.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.3jl5aovn8d (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.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/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.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=17, blended=3043, bad_region=1, passed=51550
Got 51550 stars (including 48424 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat
util/solve_plate_with_UCAC5 got 51550 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4720 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4700 matched stars entering correct_measured_positions(), 4700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4700 matched stars entering correct_measured_positions(), 51550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4720 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4700 matched stars entering correct_measured_positions(), 51550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4700 matched stars entering correct_measured_positions(), 51550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4700 stars left (next iteration limit 5170)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits N_match=4700 sigma_overall_arcsec=0.449 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.622 sigma_q3_arcsec=0.373 sigma_q4_arcsec=0.566 n_q1=1120 n_q2=1278 n_q3=1031 n_q4=1271 worst_quadrant_to_overall_ratio=1.385
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits -region wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.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.C5cVVYzRAl (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_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.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_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.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=1, no_mag_err=0, low_SNR=6, blended=1125, bad_region=1, passed=32545
Got 32545 stars (including 31366 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat
util/solve_plate_with_UCAC5 got 32545 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (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 -4.2)
Done reading UCAC5 zone files...
Matched 4750 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4725 matched stars entering correct_measured_positions(), 4726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4724 matched stars entering correct_measured_positions(), 32545 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 -4.2)
Done reading UCAC5 zone files...
Matched 4750 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4725 matched stars entering correct_measured_positions(), 32545 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4724 matched stars entering correct_measured_positions(), 32545 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4724 stars left (next iteration limit 5196)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4724 robust_rms=9.249 arcsec worst_quadrant_rms=16.993 arcsec
SIP_REFIT: SIP order 3 trial: matched=4724 robust_rms=0.405 arcsec worst_quadrant_rms=0.414 arcsec
SIP_REFIT: SIP order 5 trial: matched=4724 robust_rms=0.276 arcsec worst_quadrant_rms=0.303 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4724 robust_rms_before=0.916 arcsec robust_rms_before_corrected=0.288 arcsec robust_rms_after=0.276 arcsec worst_quadrant_rms_before=0.307 worst_quadrant_rms_after=0.303
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.307 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits N_match=4724 sigma_overall_arcsec=0.292 sigma_q1_arcsec=0.308 sigma_q2_arcsec=0.309 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.269 n_q1=1350 n_q2=975 n_q3=1385 n_q4=1014 worst_quadrant_to_overall_ratio=1.059
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.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.5mE1ZfsxBF (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_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.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_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.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=1, no_mag_err=0, low_SNR=12, blended=1029, bad_region=1, passed=32419
Got 32419 stars (including 31323 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat
util/solve_plate_with_UCAC5 got 32419 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (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 -4.2)
Done reading UCAC5 zone files...
Matched 4743 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4716 matched stars entering correct_measured_positions(), 4716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4716 matched stars entering correct_measured_positions(), 32419 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 -15.5 to -4.2)
Done reading UCAC5 zone files...
Matched 4744 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4714 matched stars entering correct_measured_positions(), 32419 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4714 matched stars entering correct_measured_positions(), 32419 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4714 stars left (next iteration limit 5187)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4714 robust_rms=9.531 arcsec worst_quadrant_rms=16.148 arcsec
SIP_REFIT: SIP order 3 trial: matched=4714 robust_rms=0.409 arcsec worst_quadrant_rms=0.433 arcsec
SIP_REFIT: SIP order 5 trial: matched=4714 robust_rms=0.272 arcsec worst_quadrant_rms=0.300 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4714 robust_rms_before=0.917 arcsec robust_rms_before_corrected=0.286 arcsec robust_rms_after=0.272 arcsec worst_quadrant_rms_before=0.327 worst_quadrant_rms_after=0.300
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.327 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits N_match=4714 sigma_overall_arcsec=0.288 sigma_q1_arcsec=0.295 sigma_q2_arcsec=0.319 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.269 n_q1=1330 n_q2=980 n_q3=1381 n_q4=1023 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.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_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.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_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-43-26_20.00sec_0.00C_LIGHTs_0212.fits
Saving fully-calibrated image wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.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_2026-08-24_CI_Aqr-03-Q1b1x1_004741_TTUQ1b1x1_2621896_49jeC1tk/wcs_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213.fits
Preparing the HTML report for the field Aqr-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:28:46.31 -13:01:32.0: 13.91 +/- 0.08 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:03:57.95 -08:40:38.9: 12.92 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:05:33.50 -06:34:35.7: 13.04 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:45:12.59 -06:20:41.9: 13.19 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:32:44.25 -09:18:58.3: 12.52 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:17:23.56 -10:32:58.7: 12.51 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 20:57:56.16 -08:21:39.1: 13.05 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:33:18.30 -07:01:40.6: 13.50 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:21:36.56 -08:36:45.3: 13.94 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:38:57.92 -08:15:41.8: 12.87 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:03:57.95 -08:40:38.9: 13.02 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:28:46.31 -13:01:32.0: 13.91 +/- 0.08 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:45:12.59 -06:20:41.9: 13.21 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:05:33.50 -06:34:35.7: 13.02 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:17:23.56 -10:32:58.7: 12.36 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:32:44.25 -09:18:58.3: 12.50 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:21:36.56 -08:36:45.3: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry reference-image weighted average: 13.91 +/- 0.06
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 20:57:56.16 -08:21:39.1: 13.17 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:33:18.30 -07:01:40.6: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter REJECTED candidate at 21:03:57.95 -08:40:38.9: ref_mag=12.97 +/- 0.02 new_mean_mag=13.2921 delta=-0.33 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:38:57.92 -08:15:41.8: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter REJECTED candidate at 21:45:12.59 -06:20:41.9: ref_mag=13.20 +/- 0.03 new_mean_mag=13.2729 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:28:46.31 -13:01:32.0: ref_mag=13.91 +/- 0.06 new_mean_mag=13.9461 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:05:33.50 -06:34:35.7: ref_mag=13.03 +/- 0.02 new_mean_mag=13.1309 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Forced photometry filter REJECTED candidate at 21:17:23.56 -10:32:58.7: ref_mag=12.42 +/- 0.01 new_mean_mag=12.9086 delta=-0.49 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:32:44.25 -09:18:58.3: ref_mag=12.51 +/- 0.01 new_mean_mag=13.1408 delta=-0.63 (need > 0.90)
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter REJECTED candidate at 21:21:36.56 -08:36:45.3: ref_mag=13.88 +/- 0.05 new_mean_mag=13.9589 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter REJECTED candidate at 21:33:18.30 -07:01:40.6: ref_mag=13.41 +/- 0.03 new_mean_mag=13.5046 delta=-0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 20:57:56.16 -08:21:39.1: ref_mag=13.11 +/- 0.03 new_mean_mag=13.2249 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:38:57.92 -08:15:41.8: ref_mag=12.88 +/- 0.02 new_mean_mag=12.9997 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:03:37.34 -12:20:39.6: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:00:28.69 -05:46:36.1: 13.43 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:13:40.34 -14:39:06.5: 13.07 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:34:15.36 -06:17:37.4: 11.43 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:00:49.20 -05:23:56.8: 12.52 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:07:40.27 -05:33:59.8: 13.45 +/- 0.06 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:32:22.79 -12:17:28.2: 13.20 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:01:25.98 -07:25:41.2: 13.27 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:36:45.98 -12:19:23.5: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:03:37.34 -12:20:39.6: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:07:40.27 -05:33:59.8: 13.69 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:00:49.20 -05:23:56.8: 12.67 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:34:15.36 -06:17:37.4: 11.38 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:32:22.79 -12:17:28.2: 13.18 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:13:40.34 -14:39:06.5: 13.10 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:00:28.69 -05:46:36.1: 13.86 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Forced photometry reference-image weighted average: 11.41 +/- 0.01
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry reference-image weighted average: 13.59 +/- 0.05
Forced photometry filter REJECTED candidate at 21:07:40.27 -05:33:59.8: ref_mag=13.56 +/- 0.04 new_mean_mag=13.5861 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:00:49.20 -05:23:56.8: ref_mag=12.60 +/- 0.02 new_mean_mag=12.6274 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:32:22.79 -12:17:28.2: ref_mag=13.19 +/- 0.03 new_mean_mag=13.2377 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:34:15.36 -06:17:37.4: ref_mag=11.41 +/- 0.01 new_mean_mag=11.7274 delta=-0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:13:40.34 -14:39:06.5: ref_mag=13.08 +/- 0.03 new_mean_mag=13.1712 delta=-0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:00:28.69 -05:46:36.1: ref_mag=13.59 +/- 0.05 new_mean_mag=13.6007 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:53:54.71 -13:19:59.7: 15.28 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:01:25.98 -07:25:41.2: 13.15 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:36:45.98 -12:19:23.5: 15.52 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter REJECTED candidate at 21:01:25.98 -07:25:41.2: ref_mag=13.20 +/- 0.03 new_mean_mag=13.4691 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:53:54.71 -13:19:59.7: 15.19 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:36:18.35 -05:33:17.9: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:22:54.01 -12:45:24.1: 13.82 +/- 0.07 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:22:22.94 -06:35:23.8: 13.52 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-06-18_04-19-51_20.00sec_5.00C_LIGHT_0387.fits at 21:45:31.15 -08:01:46.8: 13.47 +/- 0.05 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:22:22.94 -06:35:23.8: 13.65 +/- 0.06 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:36:18.35 -05:33:17.9: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:22:54.01 -12:45:24.1: 13.97 +/- 0.08 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-07-17_03-50-11_20.00sec_5.00C_LIGHT_0198.fits at 21:45:31.15 -08:01:46.8: 13.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.04
Forced photometry reference-image weighted average: 13.88 +/- 0.06
Forced photometry filter REJECTED candidate at 21:22:22.94 -06:35:23.8: ref_mag=13.58 +/- 0.04 new_mean_mag=13.6606 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.49 +/- 0.04
Forced photometry filter REJECTED candidate at 21:22:54.01 -12:45:24.1: ref_mag=13.88 +/- 0.06 new_mean_mag=13.7933 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:45:31.15 -08:01:46.8: ref_mag=13.49 +/- 0.04 new_mean_mag=13.7023 delta=-0.22 (need > 0.90)
Adding exclusion_list_local.txt__out68572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69164.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68120_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68120_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68121_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68121_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68124_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68124_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68125_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68125_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68126_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68126_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68129_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68129_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68130_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68130_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68131_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68131_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68132_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68132_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68133_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68133_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68135_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68135_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68271_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68271_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
**** FOUND 21:05:40.66 -08:05:24.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68544_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68544_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
**** FOUND 21:31:37.71 -05:36:32.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68545_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68545_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68572_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
Preparing report for the candidate 68572_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68665_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68665_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
**** FOUND 21:31:38.56 -05:36:58.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68884_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68884_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68900_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68900_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68985_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 68985_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69046_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 69046_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69055_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 69055_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69063_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 69063_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
**** FOUND 21:45:00.05 -09:03:13.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69107_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
Preparing report for the candidate 69107_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69157_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
Preparing report for the candidate 69157_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69164_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
Preparing report for the candidate 69164_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69200_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 69200_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69277_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 69277_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69280_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 69280_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69282_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 69282_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
**** FOUND 21:19:05.53 -11:11:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65100_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 65100_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
**** FOUND 21:15:02.83 -09:46:37.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49245_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213
The candidate 49245_fd_Aqr-03-Q1b1x1_2026-08-24_00-44-12_20.00sec_-0.00C_LIGHTs_0213 did not pass the final checks
