This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 03.4280 2461255.9280 9.63 23:01:13.30 -15:54:39.1
50.96087 -62.10621 galactic Aqr Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.9 Metis -0 -0 0 9.7 -0 -0
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:01:13.30 -15:54:39.1: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:01:13.30 -15:54:39.1: 14.76 +/- 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,2461255.9280,9.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.4280 9.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4280 2461255.9280 12.44 23:11:40.64 -20:53:57.6
42.83558 -66.42883 galactic Aqr Second-epoch detections are separated by 0.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1021 Flammario -0 0 0 12.4 -0 -0
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:11:40.64 -20:53:57.6: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:11:40.64 -20:53:57.6: 14.76 +/- 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,2461255.9280,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.4280 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4280 2461255.9280 13.79 22:48:04.96 -20:06:51.6
40.22124 -60.96913 galactic Aqr Second-epoch detections are separated by 2.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.278 Paulina -1 1 2 13.8 0 0
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 22:48:04.96 -20:06:51.6: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 22:48:04.96 -20:06:51.6: 14.77 +/- 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,2461255.9280,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.4280 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4280 2461255.9280 10.75 22:57:06.68 -20:20:34.3
41.30809 -63.03744 galactic Aqr Second-epoch detections are separated by 0.5" and 5.0 pix
The object was found in VSX 3" S Aqr
Type: M
# Max. Min./Amp. JD0 Period
7.600 V 15.000 V 2452107.00000 279.300000000000 M4e-M6e
The object was not found in astcheck.
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 22:57:06.68 -20:20:34.3: 11.70 +/- 0.02 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 22:57:06.68 -20:20:34.3: 11.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
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
S Aqr,2461255.9280,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
S Aqr 20260803.4280 10.75CV 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: 2461212.88469579 21.06.2026 09:13:47.716 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
First image: 2461212.88469579 21.06.2026 09:13:47.716 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Last image: 2461255.92829370 03.08.2026 10:16:34.576 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.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.: -8.18
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 2592
Objects passed selection criteria: 2581
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 2086.75
Average stars matched: 1952 (93.5426 %)
Memory usage VmPeak: 229492 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 3 05:26:36 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: 2461212.88469579 21.06.2026 09:13:47.716 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
First image: 2461212.88469579 21.06.2026 09:13:47.716 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Last image: 2461255.92829370 03.08.2026 10:16:34.576 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 25
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.86
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: 11 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 17235
Objects passed selection criteria: 17180
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 14010.5
Average stars matched: 13031 (93.0088 %)
Memory usage VmPeak: 241216 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 3 05:27:23 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
SExtractor catalog cache: saved Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.cat to cache
SExtractor catalog cache: saved Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.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: 2461255.92771679
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits exists and is non-empty
Saving wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits to local_wcs_cache/
'wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits' -> 'local_wcs_cache/wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits'
wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits exists and is non-empty
Saving wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits to local_wcs_cache/
'wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits' -> 'local_wcs_cache/wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits'
wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits exists and is non-empty
Saving wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits to local_wcs_cache/
'wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits' -> 'local_wcs_cache/wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits'
wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits exists and is non-empty
Saving wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits to local_wcs_cache/
'wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits' -> 'local_wcs_cache/wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (1st reference image)
verification OK: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Image size: 937.7'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 23:06:40.465 -17:59:46.14 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits (1st new image)
verification OK: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
Image size: 937.2'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:40.923 -18:00:17.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:40.465 -17:59:46.14
Second-epoch image center 23:06:40.923 -18:00:17.30
Angular distance between the image centers 0.0088 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits (2nd new image)
verification OK: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Image size: 937.2'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:39.843 -18:00:41.80 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:40.465 -17:59:46.14
Second-epoch image center 23:06:39.843 -18:00:41.80
Angular distance between the image centers 0.0157 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 23:06:40.923 -18:00:17.30
Second-epoch second image center 23:06:39.843 -18:00:41.80
Angular distance between the image centers 0.00804 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits &> /tmp/tmp.fZEnL2xTcD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits &> /tmp/tmp.jOAI5cKE1A
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits &> /tmp/tmp.eWQWVTEBC5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits &> /tmp/tmp.7jqMjuc0xo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
Found non-empty wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
The reference image (wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits) and catalog (wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat) found
'wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat' -> 'wcsmag.cat'
Read 3335 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2681 to 355.1405 deg, Dec -23.2523 to -12.5761 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 338.2681 to 355.1405 deg, Dec -23.2523 to -12.5761 deg
Loaded 4546 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): 2669 out of 2711 total matches.
Matched with Tycho-2 2711 out of 3335 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.435500
a=0.000000 b=1.000000 c=22.435500
From vast_summary.log: estimated ref. image limiting mag.: -8.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.26
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 3335 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2681 to 355.1405 deg, Dec -23.2523 to -12.5761 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 338.2681 to 355.1405 deg, Dec -23.2523 to -12.5761 deg
Loaded 4546 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): 2669 out of 2711 total matches.
Matched with Tycho-2 2711 out of 3335 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Forced-photometry filter: calibrated wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits -> calib.txt_param_ref_wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (aperture=6.2)
Read 2735 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2677 to 355.1377 deg, Dec -23.2523 to -12.5973 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 338.2677 to 355.1377 deg, Dec -23.2523 to -12.5973 deg
Loaded 4533 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): 2231 out of 2254 total matches.
Matched with Tycho-2 2254 out of 2735 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Forced-photometry filter: calibrated wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits -> calib.txt_param_ref_wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
2.2 pix Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
2.2 pix fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
2.2 pix fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Limiting magnitude estimates:
14.3 mag. Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
14.0 mag. Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
13.9 mag. fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
13.9 mag. fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.fZEnL2xTcD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits' -> 'wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS-calibrated image found: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Checking if the catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS catalog name: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=238, bad_region=696, passed=3335
Got 3335 stars (including 2446 good ones) from the SExtractor catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
util/solve_plate_with_UCAC5 got 3335 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 2317 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2312 matched stars entering correct_measured_positions(), 2312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2312 matched stars entering correct_measured_positions(), 2761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 2317 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2311 matched stars entering correct_measured_positions(), 2761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 2311 matched stars entering correct_measured_positions(), 2760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 2311 stars left (next iteration limit 2543)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits N_match=2311 sigma_overall_arcsec=0.367 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.390 sigma_q4_arcsec=0.350 n_q1=783 n_q2=386 n_q3=710 n_q4=432 worst_quadrant_to_overall_ratio=1.064
The image catalog is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits -region wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.jOAI5cKE1A (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits' -> 'wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS_IMAGE_NAME=wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS-calibrated image found: wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Checking if the catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits alredy exist and is non-empty...
Catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS catalog name: wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=193, bad_region=579, passed=2735
Got 2735 stars (including 2002 good ones) from the SExtractor catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 2735 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 1902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1900 matched stars entering correct_measured_positions(), 1900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1900 matched stars entering correct_measured_positions(), 2242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 1902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1900 matched stars entering correct_measured_positions(), 2242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 1900 matched stars entering correct_measured_positions(), 2242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 1900 stars left (next iteration limit 2090)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits N_match=1900 sigma_overall_arcsec=0.387 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.471 sigma_q4_arcsec=0.344 n_q1=625 n_q2=315 n_q3=613 n_q4=347 worst_quadrant_to_overall_ratio=1.217
The image catalog is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits -region wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eWQWVTEBC5 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
WCS-calibrated image found: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
Checking if the catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
WCS catalog name: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=262, bad_region=621, passed=2424
Got 2424 stars (including 1583 good ones) from the SExtractor catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat
util/solve_plate_with_UCAC5 got 2424 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 1518 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1514 matched stars entering correct_measured_positions(), 1514 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1514 matched stars entering correct_measured_positions(), 1897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 1518 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1515 matched stars entering correct_measured_positions(), 1897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 1515 matched stars entering correct_measured_positions(), 1897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 1515 stars left (next iteration limit 1665)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1515 robust_rms=6.590 arcsec worst_quadrant_rms=7.963 arcsec
SIP_REFIT: SIP order 3 trial: matched=1515 robust_rms=0.366 arcsec worst_quadrant_rms=0.437 arcsec
SIP_REFIT: SIP order 5 trial: matched=1515 robust_rms=0.287 arcsec worst_quadrant_rms=0.301 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1515 robust_rms_before=0.996 arcsec robust_rms_before_corrected=0.310 arcsec robust_rms_after=0.287 arcsec worst_quadrant_rms_before=0.319 worst_quadrant_rms_after=0.301
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.319 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits N_match=1515 sigma_overall_arcsec=0.307 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.315 sigma_q3_arcsec=0.311 sigma_q4_arcsec=0.291 n_q1=465 n_q2=304 n_q3=447 n_q4=299 worst_quadrant_to_overall_ratio=1.023
The image catalog is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits -region wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.7jqMjuc0xo (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
WCS-calibrated image found: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Checking if the catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
WCS catalog name: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=297, bad_region=610, passed=2435
Got 2435 stars (including 1575 good ones) from the SExtractor catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat
util/solve_plate_with_UCAC5 got 2435 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 1510 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1509 matched stars entering correct_measured_positions(), 1509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1509 matched stars entering correct_measured_positions(), 1909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 1510 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1509 matched stars entering correct_measured_positions(), 1909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 1509 matched stars entering correct_measured_positions(), 1909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 1509 stars left (next iteration limit 1659)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1509 robust_rms=6.694 arcsec worst_quadrant_rms=8.097 arcsec
SIP_REFIT: SIP order 3 trial: matched=1509 robust_rms=0.422 arcsec worst_quadrant_rms=0.466 arcsec
SIP_REFIT: SIP order 5 trial: matched=1509 robust_rms=0.337 arcsec worst_quadrant_rms=0.365 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1509 robust_rms_before=0.989 arcsec robust_rms_before_corrected=0.351 arcsec robust_rms_after=0.337 arcsec worst_quadrant_rms_before=0.370 worst_quadrant_rms_after=0.365
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.370 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits N_match=1509 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.345 sigma_q2_arcsec=0.413 sigma_q3_arcsec=0.339 sigma_q4_arcsec=0.335 n_q1=460 n_q2=303 n_q3=452 n_q4=294 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits -region wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits sigma_overall=0.367 worst_q_ratio=1.064
ref2=Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits sigma_overall=0.387 worst_q_ratio=1.217
new1=fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits sigma_overall=0.307 worst_q_ratio=1.023
new2=fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits sigma_overall=0.362 worst_q_ratio=1.142
reference average sigma_overall=0.377 worst_q_ratio=1.1405
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406_astrometric_residuals.png (2311 matched stars from wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410_astrometric_residuals.png (1900 matched stars from wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480_astrometric_residuals.png (1515 matched stars from wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481_astrometric_residuals.png (1509 matched stars from wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits'
Saving fully-calibrated image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits'
Preparing the HTML report for the field Aqr-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 22:57:06.65 -20:20:34.8: 11.50 +/- 0.02 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:01:13.30 -15:54:39.1: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 22:57:06.65 -20:20:34.8: 11.59 +/- 0.02 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:01:13.30 -15:54:39.1: 14.76 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.53 +/- 0.01
Forced photometry filter KEPT candidate at 22:57:06.65 -20:20:34.8: ref_mag=11.53 +/- 0.01 new_mean_mag=10.5749 delta=0.96 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out00931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20135.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 20135_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
Preparing report for the candidate 20135_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00931_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 00931_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
**** FOUND 22:57:06.65 -20:20:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.57, MAG_FAINT_SEARCH_LIMIT=11.55)GAIADR2_OUTPUT=# 2.432 2399318338141987200 344.27704916341 -20.34327299756 9.1620 7.6031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Aqr-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:01:13.30 -15:54:39.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
SExtractor catalog cache: saved Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.cat to cache
SExtractor catalog cache: saved Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Creating symlink local_wcs_cache/wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits exists and is non-empty
wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits exists and is non-empty
wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits exists and is non-empty
wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (1st reference image)
verification OK: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Image size: 937.7'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 23:06:40.465 -17:59:46.14 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits (1st new image)
verification OK: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
Image size: 937.2'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:40.923 -18:00:17.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:40.465 -17:59:46.14
Second-epoch image center 23:06:40.923 -18:00:17.30
Angular distance between the image centers 0.0088 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits (2nd new image)
verification OK: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Image size: 937.2'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:39.843 -18:00:41.80 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:40.465 -17:59:46.14
Second-epoch image center 23:06:39.843 -18:00:41.80
Angular distance between the image centers 0.0157 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 23:06:40.923 -18:00:17.30
Second-epoch second image center 23:06:39.843 -18:00:41.80
Angular distance between the image centers 0.00804 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits &> /tmp/tmp.sfQp3HlN7K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits &> /tmp/tmp.TXuVAO0Qqt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits &> /tmp/tmp.x9egOEneFO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits &> /tmp/tmp.2C4mBSwEYY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
Found non-empty wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits and wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
The reference image (wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits) and catalog (wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat) found
'wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat' -> 'wcsmag.cat'
Read 19454 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2356 to 355.1719 deg, Dec -23.2559 to -12.5761 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 338.2356 to 355.1719 deg, Dec -23.2559 to -12.5761 deg
Loaded 4568 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): 3693 out of 3823 total matches.
Matched with Tycho-2 3823 out of 19454 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.293600
a=0.000000 b=1.000000 c=22.293600
From vast_summary.log: estimated ref. image limiting mag.: -7.86
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 19454 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2356 to 355.1719 deg, Dec -23.2559 to -12.5761 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 338.2356 to 355.1719 deg, Dec -23.2559 to -12.5761 deg
Loaded 4568 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): 3693 out of 3823 total matches.
Matched with Tycho-2 3823 out of 19454 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Forced-photometry filter: calibrated wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits -> calib.txt_param_ref_wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits (aperture=4.8)
Read 17815 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.2344 to 355.1739 deg, Dec -23.2554 to -12.5760 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 338.2344 to 355.1739 deg, Dec -23.2554 to -12.5760 deg
Loaded 4568 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): 3728 out of 3836 total matches.
Matched with Tycho-2 3836 out of 17815 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Forced-photometry filter: calibrated wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits -> calib.txt_param_ref_wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
2.1 pix Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
2.1 pix fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
2.1 pix fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Limiting magnitude estimates:
14.4 mag. Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
14.2 mag. Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
14.0 mag. fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
14.1 mag. fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.sfQp3HlN7K (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.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-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits' -> 'wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS-calibrated image found: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
Checking if the catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits
WCS catalog name: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=650, bad_region=2800, passed=19446
Got 19446 stars (including 16167 good ones) from the SExtractor catalog wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat
util/solve_plate_with_UCAC5 got 19446 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4784 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 4778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 17350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4784 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 17350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 17350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4778 stars left (next iteration limit 5255)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits N_match=4778 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.392 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.362 n_q1=1568 n_q2=774 n_q3=1522 n_q4=914 worst_quadrant_to_overall_ratio=1.034
The image catalog is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits -region wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TXuVAO0Qqt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.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-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits' -> 'wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS_IMAGE_NAME=wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS-calibrated image found: wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
Checking if the catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits alredy exist and is non-empty...
Catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat corresponding to the image wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits
WCS catalog name: wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=542, bad_region=2798, passed=17807
Got 17807 stars (including 14549 good ones) from the SExtractor catalog wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 17807 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4789 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 4782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 15700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4789 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 15700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 15700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4782 stars left (next iteration limit 5260)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits N_match=4782 sigma_overall_arcsec=0.415 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.423 sigma_q3_arcsec=0.469 sigma_q4_arcsec=0.368 n_q1=1572 n_q2=818 n_q3=1474 n_q4=918 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits -region wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.x9egOEneFO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
WCS-calibrated image found: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
Checking if the catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
WCS catalog name: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=3, no_mag_err=0, low_SNR=2, blended=425, bad_region=2855, passed=15154
Got 15154 stars (including 11981 good ones) from the SExtractor catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat
util/solve_plate_with_UCAC5 got 15154 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4836 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 4830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 12971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4834 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 12971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 12971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4830 stars left (next iteration limit 5313)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits N_match=4830 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.374 sigma_q2_arcsec=0.365 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.378 n_q1=1532 n_q2=962 n_q3=1438 n_q4=898 worst_quadrant_to_overall_ratio=1.021
The image catalog is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits -region wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2C4mBSwEYY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
WCS-calibrated image found: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Checking if the catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat corresponding to the image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
WCS catalog name: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=470, bad_region=2867, passed=15344
Got 15344 stars (including 12123 good ones) from the SExtractor catalog wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat
util/solve_plate_with_UCAC5 got 15344 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4839 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 4832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 13158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4837 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 13158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 13158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4832 stars left (next iteration limit 5315)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits N_match=4832 sigma_overall_arcsec=0.421 sigma_q1_arcsec=0.404 sigma_q2_arcsec=0.425 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.425 n_q1=1555 n_q2=948 n_q3=1449 n_q4=880 worst_quadrant_to_overall_ratio=1.025
The image catalog is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits -region wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-15-44_20.00sec_-0.00C_LIGHT_0480.fits
Saving fully-calibrated image wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aqr-07-Q2b1x1_052309_TTUQ2b1x1_365751_4DMtvlQ6/wcs_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481.fits
Preparing the HTML report for the field Aqr-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:23:26.20 -21:30:31.1: 13.84 +/- 0.16 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:24:11.62 -14:55:24.0: 13.23 +/- 0.08 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:04:00.65 -20:54:25.0: 14.14 +/- 0.17 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:11:40.64 -20:53:57.6: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:20:56.46 -18:31:26.1: 13.16 +/- 0.08 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:16:59.52 -22:03:16.8: 13.97 +/- 0.17 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 22:48:04.96 -20:06:51.6: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:24:18.07 -22:08:58.8: 14.02 +/- 0.18 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:24:10.24 -20:45:07.8: 13.86 +/- 0.15 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 22:56:07.39 -21:34:02.7: 14.31 +/- 0.21 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:23:26.20 -21:30:31.1: 13.84 +/- 0.18 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:24:11.62 -14:55:24.0: 13.21 +/- 0.09 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:11:40.64 -20:53:57.6: 14.76 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:20:56.46 -18:31:26.1: 13.05 +/- 0.08 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:16:59.52 -22:03:16.8: 14.02 +/- 0.21 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:04:00.65 -20:54:25.0: 13.97 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.12
Forced photometry reference-image weighted average: 13.10 +/- 0.06
Forced photometry reference-image weighted average: 13.22 +/- 0.06
Forced photometry reference-image weighted average: 14.06 +/- 0.13
Forced photometry reference-image weighted average: 13.99 +/- 0.13
Forced photometry filter REJECTED candidate at 23:23:26.20 -21:30:31.1: ref_mag=13.84 +/- 0.12 new_mean_mag=13.7880 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:20:56.46 -18:31:26.1: ref_mag=13.10 +/- 0.06 new_mean_mag=13.0799 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:24:11.62 -14:55:24.0: ref_mag=13.22 +/- 0.06 new_mean_mag=13.2536 delta=-0.03 (need > 0.90)
Forced photometry filter KEPT candidate at 23:04:00.65 -20:54:25.0: ref_mag=14.06 +/- 0.13 new_mean_mag=12.9542 delta=1.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:16:59.52 -22:03:16.8: ref_mag=13.99 +/- 0.13 new_mean_mag=13.7511 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 22:48:04.96 -20:06:51.6: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:24:18.07 -22:08:58.8: 14.13 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.14
Forced photometry filter REJECTED candidate at 23:24:18.07 -22:08:58.8: ref_mag=14.06 +/- 0.14 new_mean_mag=13.8971 delta=0.16 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:24:10.24 -20:45:07.8: 14.24 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.13
Forced photometry filter REJECTED candidate at 23:24:10.24 -20:45:07.8: ref_mag=13.96 +/- 0.13 new_mean_mag=13.8515 delta=0.10 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 22:56:07.39 -21:34:02.7: 14.05 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.14
Forced photometry filter REJECTED candidate at 22:56:07.39 -21:34:02.7: ref_mag=14.17 +/- 0.14 new_mean_mag=13.9614 delta=0.21 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 23:11:27.64 -20:57:49.8: 14.29 +/- 0.20 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-21_04-13-47_20.00sec_5.00C_LIGHT_0406.fits at 22:57:06.68 -20:20:34.3: 11.70 +/- 0.02 detection
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 23:11:27.64 -20:57:49.8: 14.14 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.14
Forced photometry filter REJECTED candidate at 23:11:27.64 -20:57:49.8: ref_mag=14.22 +/- 0.14 new_mean_mag=13.9011 delta=0.32 (need > 0.90)
Forced photometry on wcs_Aqr-07-Q2b1x1_2026-06-23_04-35-24_20.00sec_4.90C_LIGHT_0410.fits at 22:57:06.68 -20:20:34.3: 11.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Forced photometry filter KEPT candidate at 22:57:06.68 -20:20:34.3: ref_mag=11.75 +/- 0.01 new_mean_mag=10.7504 delta=1.00 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out22274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23363.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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: 2s
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Considering the candidate 20834_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 20834_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
**** FOUND 23:01:13.30 -15:54:39.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 21817_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
Preparing report for the candidate 21817_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
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Considering the candidate 21984_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 21984_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 22274_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 22274_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
**** FOUND 23:04:00.65 -20:54:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.432 2398302178944146304 346.00236245466 -20.90671225442 13.3412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22466_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 22466_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
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Considering the candidate 22840_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 22840_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
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Considering the candidate 22869_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 22869_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 23263_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 23263_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
Rejecting candidate due to large distance (29.5") between the two second-epoch detections
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Considering the candidate 23346_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 23346_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
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Considering the candidate 23353_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 23353_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
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Considering the candidate 23358_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 23358_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
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Considering the candidate 23363_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
Preparing report for the candidate 23363_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
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Considering the candidate 23393_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 23393_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
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Considering the candidate 23442_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 23442_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks
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Considering the candidate 23462_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481
The candidate 23462_fd_Aqr-07-Q2b1x1_2026-08-03_05-16-34_20.00sec_0.00C_LIGHT_0481 did not pass the final checks