This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg
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 06 08.3969 2461199.8969 11.91 21:04:27.91 -09:28:13.7
39.85912 -33.80983 galactic Aqr Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.287 Nephthys -0 -1 1 12.2 -0 -0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:04:27.91 -09:28:13.7: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:04:27.91 -09:28:13.7: 15.07 +/- 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,2461199.8969,11.91,0.05,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 20260608.3969 11.91CV 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 06 08.3969 2461199.8969 12.14 21:30:43.13 -09:31:19.4
43.45839 -39.60647 galactic Cap Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.306 Unitas -1 -1 1 12.2 0 -0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:30:43.13 -09:31:19.4: 15.24 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:30:43.13 -09:31:19.4: 15.24 +/- 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 06 08.3970* 21 30 43.13 -09 31 19.4 12.1 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,2461199.8969,12.14,0.05,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 20260608.3969 12.14CV 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 06 08.3969 2461199.8969 12.48 21:46:29.20 -09:10:11.3
46.30693 -42.87290 galactic Cap Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.389 Industria -1 -1 2 12.8 0 -0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:46:29.20 -09:10:11.3: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:46:29.20 -09:10:11.3: 15.10 +/- 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 06 08.3970* 21 46 29.20 -09 10 11.3 12.5 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,2461199.8969,12.48,0.05,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 20260608.3969 12.48CV 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 06 08.3969 2461199.8969 13.46 21:15:57.78 -05:49:11.3
45.37083 -34.63191 galactic Aqr Second-epoch detections are separated by 1.8" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.490 Veritas -0 -2 2 13.9 -0 -0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:15:57.78 -05:49:11.3: 15.13 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:15:57.78 -05:49:11.3: 15.14 +/- 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,2461199.8969,13.46,0.05,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 20260608.3969 13.46CV 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: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
First image: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Last image: 2461199.89717985 08.06.2026 09:31:46.339 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.22
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: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7001
Objects passed selection criteria: 6998
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 6692
Average stars matched: 6590.75 (98.487 %)
Memory usage VmPeak: 112744 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 04:54:33 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: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
First image: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Last image: 2461199.89717985 08.06.2026 09:31:46.339 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 38
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.00
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: 33 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 35527
Objects passed selection criteria: 35484
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 33990
Average stars matched: 33010.8 (97.119 %)
Memory usage VmPeak: 137140 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 04:57:33 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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.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: 2461199.89671786
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'
Plate-solving the images
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits exists and is non-empty
Saving wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits to local_wcs_cache/
'wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits'
wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits exists and is non-empty
Saving wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits to local_wcs_cache/
'wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits'
wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits exists and is non-empty
Saving wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits'
wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits exists and is non-empty
Saving wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (1st reference image)
verification OK: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Image size: 941.9'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:33.187 -09:59:28.83 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
Image size: 940.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:38.585 -10:00:50.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:38.585 -10:00:50.65
Angular distance between the image centers 0.0317 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
Image size: 940.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:41.293 -10:00:31.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:41.293 -10:00:31.14
Angular distance between the image centers 0.0375 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 21:25:38.585 -10:00:50.65
Second-epoch second image center 21:25:41.293 -10:00:31.14
Angular distance between the image centers 0.01236 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits &> /tmp/tmp.yxGzb4u4Xt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits &> /tmp/tmp.Ofnr1ZIJ1s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits &> /tmp/tmp.RPWH7UfpEj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits &> /tmp/tmp.gn6vHMP9bx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat
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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat
Found non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat
The reference image (wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits) and catalog (wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat) found
'wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat' -> 'wcsmag.cat'
Read 7159 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 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 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 deg
Loaded 7438 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): 5084 out of 5196 total matches.
Matched with Tycho-2 5196 out of 7159 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.642150
a=0.000000 b=1.000000 c=22.642150
From vast_summary.log: estimated ref. image limiting mag.: -8.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7159 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 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 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 deg
Loaded 7438 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): 5084 out of 5196 total matches.
Matched with Tycho-2 5196 out of 7159 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (aperture=7.4)
Read 7189 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0145 to 329.5561 deg, Dec -15.5598 to -4.2276 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 313.0145 to 329.5561 deg, Dec -15.5598 to -4.2276 deg
Loaded 7439 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): 5086 out of 5190 total matches.
Matched with Tycho-2 5190 out of 7189 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits (aperture=7.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
3.3 pix Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.3 pix Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
3.7 pix fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
3.7 pix fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
3.3 pix wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.3 pix wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Limiting magnitude estimates:
14.4 mag. Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
14.4 mag. Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
14.2 mag. fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
14.2 mag. fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yxGzb4u4Xt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=329, passed=7159
Got 7159 stars (including 6821 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat
util/solve_plate_with_UCAC5 got 7159 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6931 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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits N_match=935 sigma_overall_arcsec=0.283 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.235 sigma_q4_arcsec=0.258 n_q1=280 n_q2=199 n_q3=264 n_q4=192 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -region wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Ofnr1ZIJ1s (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.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_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.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_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=325, passed=7189
Got 7189 stars (including 6859 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat
util/solve_plate_with_UCAC5 got 7189 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 935 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits N_match=935 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.318 sigma_q3_arcsec=0.262 sigma_q4_arcsec=0.253 n_q1=283 n_q2=199 n_q3=260 n_q4=193 worst_quadrant_to_overall_ratio=1.112
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -region wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.RPWH7UfpEj (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_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.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_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.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_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=308, passed=6277
Got 6277 stars (including 5964 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat
util/solve_plate_with_UCAC5 got 6277 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (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 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits N_match=934 sigma_overall_arcsec=0.333 sigma_q1_arcsec=0.419 sigma_q2_arcsec=0.342 sigma_q3_arcsec=0.293 sigma_q4_arcsec=0.236 n_q1=259 n_q2=225 n_q3=249 n_q4=201 worst_quadrant_to_overall_ratio=1.257
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.gn6vHMP9bx (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_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.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_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.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_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=303, passed=6293
Got 6293 stars (including 5986 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat
util/solve_plate_with_UCAC5 got 6293 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (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 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 6129 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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 6128 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 6129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 933 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits N_match=933 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.441 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.321 sigma_q4_arcsec=0.270 n_q1=258 n_q2=223 n_q3=249 n_q4=203 worst_quadrant_to_overall_ratio=1.260
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits sigma_overall=0.283 worst_q_ratio=1.198
ref2=Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits sigma_overall=0.286 worst_q_ratio=1.112
new1=fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits sigma_overall=0.333 worst_q_ratio=1.257
new2=fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits sigma_overall=0.350 worst_q_ratio=1.260
reference average sigma_overall=0.2845 worst_q_ratio=1.155
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385_astrometric_residuals.png (see messages above)
plot_astrometric_residuals_xy.py: numpy/matplotlib unavailable (No module named 'matplotlib') -- falling back to the C plotter
plot_astrometric_residuals_xy: PGPLOT /PNG device reported success but no file appeared at wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386_astrometric_residuals.png -- no plot produced
WARNING: no astrometric residual plot produced for wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits -- both lib/plot_astrometric_residuals_xy.py and lib/plot_astrometric_residuals_xy failed to create wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386_astrometric_residuals.png (see messages above)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits'
Saving fully-calibrated image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:13:49.25 -11:27:13.9: 11.53 +/- 0.01 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:13:49.25 -11:27:13.9: 11.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.01
Forced photometry filter REJECTED candidate at 21:13:49.25 -11:27:13.9: ref_mag=11.54 +/- 0.01 new_mean_mag=11.7838 delta=-0.24 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20317_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 20317_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
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 ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Creating symlink local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits exists and is non-empty
wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits exists and is non-empty
wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits exists and is non-empty
wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (1st reference image)
verification OK: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Image size: 941.9'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:33.187 -09:59:28.83 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
Image size: 940.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:38.585 -10:00:50.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:38.585 -10:00:50.65
Angular distance between the image centers 0.0317 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
Image size: 940.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:41.293 -10:00:31.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:41.293 -10:00:31.14
Angular distance between the image centers 0.0375 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 21:25:38.585 -10:00:50.65
Second-epoch second image center 21:25:41.293 -10:00:31.14
Angular distance between the image centers 0.01236 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits &> /tmp/tmp.ZiC8uRKivR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits &> /tmp/tmp.Cj9kPPTAwP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits &> /tmp/tmp.SzPHyqpWBW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits &> /tmp/tmp.g3JjOT2R9t
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat
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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat
Found non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat
The reference image (wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits) and catalog (wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat) found
'wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat' -> 'wcsmag.cat'
Read 36787 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 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 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 deg
Loaded 7455 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): 5625 out of 6011 total matches.
Matched with Tycho-2 6011 out of 36787 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.521200
a=0.000000 b=1.000000 c=22.521200
From vast_summary.log: estimated ref. image limiting mag.: -8.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36787 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 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 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 deg
Loaded 7455 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): 5625 out of 6011 total matches.
Matched with Tycho-2 6011 out of 36787 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (aperture=6.1)
Read 37049 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0031 to 329.5643 deg, Dec -15.5699 to -4.2276 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 313.0031 to 329.5643 deg, Dec -15.5699 to -4.2276 deg
Loaded 7455 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): 5641 out of 6012 total matches.
Matched with Tycho-2 6012 out of 37049 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
3.1 pix Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.1 pix Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
3.4 pix fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
3.4 pix fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
3.1 pix wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.1 pix wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Limiting magnitude estimates:
14.5 mag. Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
14.5 mag. Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
14.3 mag. fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
14.3 mag. fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
All-image limiting magnitude estimate: 14.3 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ZiC8uRKivR (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.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_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1449, passed=36780
Got 36780 stars (including 35283 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat
util/solve_plate_with_UCAC5 got 36780 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/util/fov_of_wcs_calibrated_image.sh: line 168: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 35505 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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 35507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 35508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits N_match=936 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.353 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.318 n_q1=272 n_q2=191 n_q3=280 n_q4=193 worst_quadrant_to_overall_ratio=1.178
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -region wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Cj9kPPTAwP (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.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_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.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_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1439, passed=37041
Got 37041 stars (including 35552 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat
util/solve_plate_with_UCAC5 got 37041 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 35884 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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 35882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 35886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 940 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits N_match=940 sigma_overall_arcsec=0.290 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.314 sigma_q3_arcsec=0.276 sigma_q4_arcsec=0.252 n_q1=274 n_q2=196 n_q3=275 n_q4=195 worst_quadrant_to_overall_ratio=1.080
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -region wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SzPHyqpWBW (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_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.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_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.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_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1285, passed=31563
Got 31563 stars (including 30248 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat
util/solve_plate_with_UCAC5 got 31563 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (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 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 30971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 30973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 30983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 931 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits N_match=931 sigma_overall_arcsec=0.342 sigma_q1_arcsec=0.421 sigma_q2_arcsec=0.358 sigma_q3_arcsec=0.315 sigma_q4_arcsec=0.244 n_q1=243 n_q2=223 n_q3=257 n_q4=208 worst_quadrant_to_overall_ratio=1.230
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.g3JjOT2R9t (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_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.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_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.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_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1259, passed=31635
Got 31635 stars (including 30339 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat
util/solve_plate_with_UCAC5 got 31635 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (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 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 30857 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
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 30860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 30869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 931 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits N_match=931 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.422 sigma_q2_arcsec=0.374 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.277 n_q1=244 n_q2=218 n_q3=257 n_q4=212 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits.cat.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_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.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_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-06_20.00sec_-0.00C_LIGHTs_0385.fits
Saving fully-calibrated image wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.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_2026-06-08_CI_Aqr-03-Q1b1x1_044929_TTUQ1b1x1_405241_6ocm1HAg/wcs_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386.fits
Preparing the HTML report for the field Aqr-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:29:33.95 -14:59:28.6: 12.38 +/- 0.03 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:15:57.78 -05:49:11.3: 15.13 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:30:43.13 -09:31:19.4: 15.24 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:55:55.89 -14:29:33.9: 13.59 +/- 0.13 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:56:09.89 -14:33:50.9: 13.98 +/- 0.18 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:15:07.12 -11:27:22.8: 13.25 +/- 0.06 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:54:39.12 -13:56:12.4: 13.71 +/- 0.14 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:50:28.01 -13:56:52.4: 13.68 +/- 0.12 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:04:27.91 -09:28:13.7: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:46:29.20 -09:10:11.3: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:15:57.78 -05:49:11.3: 15.14 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:55:55.89 -14:29:33.9: 13.58 +/- 0.13 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:30:43.13 -09:31:19.4: 15.24 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.58 +/- 0.09
Forced photometry filter REJECTED candidate at 21:55:55.89 -14:29:33.9: ref_mag=13.58 +/- 0.09 new_mean_mag=13.4557 delta=0.13 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:29:33.95 -14:59:28.6: 12.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.02
Forced photometry filter REJECTED candidate at 21:29:33.95 -14:59:28.6: ref_mag=12.37 +/- 0.02 new_mean_mag=12.5337 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:15:07.12 -11:27:22.8: 13.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.04
Forced photometry filter REJECTED candidate at 21:15:07.12 -11:27:22.8: ref_mag=13.24 +/- 0.04 new_mean_mag=13.4851 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:56:09.89 -14:33:50.9: 14.03 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.13
Forced photometry filter REJECTED candidate at 21:56:09.89 -14:33:50.9: ref_mag=14.00 +/- 0.13 new_mean_mag=13.6376 delta=0.36 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:50:28.01 -13:56:52.4: 13.64 +/- 0.11 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:54:39.12 -13:56:12.4: 13.84 +/- 0.15 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:04:27.91 -09:28:13.7: 15.07 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.66 +/- 0.08
Forced photometry reference-image weighted average: 13.77 +/- 0.10
Forced photometry filter REJECTED candidate at 21:50:28.01 -13:56:52.4: ref_mag=13.66 +/- 0.08 new_mean_mag=13.5233 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:54:39.12 -13:56:12.4: ref_mag=13.77 +/- 0.10 new_mean_mag=13.5765 delta=0.19 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:46:29.20 -09:10:11.3: 15.10 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:46:04.66 -14:25:42.0: 13.55 +/- 0.11 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:55:53.84 -10:04:10.5: 14.06 +/- 0.16 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:52:23.10 -14:28:16.5: 13.67 +/- 0.13 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:56:34.17 -06:41:58.4: 13.83 +/- 0.14 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:50:58.16 -10:02:03.0: 13.82 +/- 0.13 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:43:14.05 -12:54:47.0: 13.87 +/- 0.12 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:55:53.84 -10:04:10.5: 14.18 +/- 0.18 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:46:04.66 -14:25:42.0: 13.71 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.12
Forced photometry filter REJECTED candidate at 21:55:53.84 -10:04:10.5: ref_mag=14.11 +/- 0.12 new_mean_mag=13.7506 delta=0.36 (need > 0.90)
Forced photometry reference-image weighted average: 13.62 +/- 0.08
Forced photometry filter REJECTED candidate at 21:46:04.66 -14:25:42.0: ref_mag=13.62 +/- 0.08 new_mean_mag=13.6456 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:56:34.17 -06:41:58.4: 14.48 +/- 0.25 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:52:23.10 -14:28:16.5: 13.88 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.12
Forced photometry filter REJECTED candidate at 21:56:34.17 -06:41:58.4: ref_mag=13.99 +/- 0.12 new_mean_mag=13.8831 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.76 +/- 0.10
Forced photometry filter REJECTED candidate at 21:52:23.10 -14:28:16.5: ref_mag=13.76 +/- 0.10 new_mean_mag=13.7717 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:50:58.16 -10:02:03.0: 13.84 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.09
Forced photometry filter REJECTED candidate at 21:50:58.16 -10:02:03.0: ref_mag=13.83 +/- 0.09 new_mean_mag=13.6907 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:43:14.05 -12:54:47.0: 13.95 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.09
Forced photometry filter REJECTED candidate at 21:43:14.05 -12:54:47.0: ref_mag=13.90 +/- 0.09 new_mean_mag=13.5806 delta=0.32 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:46:17.28 -06:36:22.4: 13.99 +/- 0.14 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:51:44.05 -07:44:55.6: 14.26 +/- 0.19 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:51:26.13 -13:24:17.5: 14.09 +/- 0.17 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:54:45.59 -12:27:48.7: 13.96 +/- 0.16 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:46:17.28 -06:36:22.4: 14.30 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.11
Forced photometry filter REJECTED candidate at 21:46:17.28 -06:36:22.4: ref_mag=14.11 +/- 0.11 new_mean_mag=13.8726 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:51:44.05 -07:44:55.6: 14.34 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.14
Forced photometry filter REJECTED candidate at 21:51:44.05 -07:44:55.6: ref_mag=14.30 +/- 0.14 new_mean_mag=13.9852 delta=0.31 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:54:45.59 -12:27:48.7: 13.98 +/- 0.16 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:48:13.62 -12:06:51.5: 13.96 +/- 0.14 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:25:40.65 -14:49:11.7: 13.86 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.11
Forced photometry filter REJECTED candidate at 21:54:45.59 -12:27:48.7: ref_mag=13.97 +/- 0.11 new_mean_mag=13.8051 delta=0.16 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:25:40.65 -14:49:11.7: 13.88 +/- 0.13 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:51:26.13 -13:24:17.5: 13.98 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.12
Forced photometry reference-image weighted average: 13.87 +/- 0.09
Forced photometry filter REJECTED candidate at 21:51:26.13 -13:24:17.5: ref_mag=14.03 +/- 0.12 new_mean_mag=13.9918 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:25:40.65 -14:49:11.7: ref_mag=13.87 +/- 0.09 new_mean_mag=13.7984 delta=0.08 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:48:13.62 -12:06:51.5: 13.94 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.10
Forced photometry filter REJECTED candidate at 21:48:13.62 -12:06:51.5: ref_mag=13.95 +/- 0.10 new_mean_mag=13.7764 delta=0.18 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:52:42.34 -12:59:37.9: 13.92 +/- 0.15 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:42:45.53 -12:55:54.3: 14.01 +/- 0.14 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:52:42.34 -12:59:37.9: 13.87 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.10
Forced photometry filter REJECTED candidate at 21:52:42.34 -12:59:37.9: ref_mag=13.89 +/- 0.10 new_mean_mag=13.7010 delta=0.19 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:36:37.15 -13:19:45.9: 14.08 +/- 0.15 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:17:59.72 -13:47:49.7: 14.06 +/- 0.15 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:45:49.49 -05:55:49.6: 14.48 +/- 0.22 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:42:45.53 -12:55:54.3: 13.93 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.10
Forced photometry filter REJECTED candidate at 21:42:45.53 -12:55:54.3: ref_mag=13.97 +/- 0.10 new_mean_mag=14.0147 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:25:12.29 -13:39:44.5: 13.92 +/- 0.13 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:17:59.72 -13:47:49.7: 13.98 +/- 0.13 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:36:37.15 -13:19:45.9: 14.02 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.10
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:25:12.29 -13:39:44.5: 14.18 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.10
Forced photometry filter REJECTED candidate at 21:17:59.72 -13:47:49.7: ref_mag=14.02 +/- 0.10 new_mean_mag=13.8123 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:36:37.15 -13:19:45.9: ref_mag=14.05 +/- 0.10 new_mean_mag=13.8473 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 14.02 +/- 0.10
Forced photometry filter REJECTED candidate at 21:25:12.29 -13:39:44.5: ref_mag=14.02 +/- 0.10 new_mean_mag=13.9428 delta=0.08 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:45:49.49 -05:55:49.6: 14.35 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.14
Forced photometry filter REJECTED candidate at 21:45:49.49 -05:55:49.6: ref_mag=14.40 +/- 0.14 new_mean_mag=14.0248 delta=0.38 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:24:18.08 -15:04:09.3: 13.70 +/- 0.11 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:24:18.08 -15:04:09.3: 13.80 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.08
Forced photometry filter REJECTED candidate at 21:24:18.08 -15:04:09.3: ref_mag=13.74 +/- 0.08 new_mean_mag=13.8828 delta=-0.14 (need > 0.90)
Adding exclusion_list_local.txt__out53004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53068.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 52977_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 52977_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 52986_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 52986_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53004_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
Preparing report for the candidate 53004_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
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Considering the candidate 53007_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
Preparing report for the candidate 53007_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
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Considering the candidate 53017_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
Preparing report for the candidate 53017_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
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Considering the candidate 53049_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53049_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53053_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53053_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53060_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53060_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53064_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53064_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53068_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
Preparing report for the candidate 53068_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
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Considering the candidate 53071_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53071_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53076_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53076_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53077_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53077_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53081_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53081_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53099_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53099_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53100_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53100_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53106_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53106_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53107_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53107_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53118_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53118_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53120_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53120_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53121_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53121_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53123_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53123_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53132_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53132_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53145_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53145_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53148_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53148_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53149_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53149_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53166_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53166_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53186_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53186_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks
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Considering the candidate 53192_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386
The candidate 53192_fd_Aqr-03-Q1b1x1_2026-06-08_04-31-46_20.00sec_-0.00C_LIGHTs_0386 did not pass the final checks