This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 08.3524 2461291.8524 14.20 22:36:50.11 -00:05:48.4
67.23695 -47.86986 galactic Aqr Second-epoch detections are separated by 1.4" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1023 Thomana 1 -0 1 14.3 -0 -0
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:36:50.11 -00:05:48.4: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:36:50.11 -00:05:48.4: 15.84 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461291.8524,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260908.3524 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 08.3524 2461291.8524 14.48 22:12:26.18 +02:05:08.1
63.85091 -41.85198 galactic Aqr Second-epoch detections are separated by 3.4" and 10.2 pix This object is listed in spacecraft.txt 27.4" JWST
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:12:26.18 +02:05:08.1 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:12:26.18 +02:05:08.1: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:12:26.18 +02:05:08.1: 15.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461291.8524,14.48,0.05,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
target 20260908.3524 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 08.3524 2461291.8524 14.61 22:08:45.64 -04:57:24.7
55.33637 -45.39104 galactic Aqr Second-epoch detections are separated by 2.2" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.854 Frostia -2 -0 2 14.5 0 0
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:08:45.64 -04:57:24.7: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:08:45.64 -04:57:24.7: 15.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461291.8524,14.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260908.3524 14.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 08.3524 2461291.8524 14.35 22:03:57.01 -03:09:06.8
56.45439 -43.37641 galactic Aqr Second-epoch detections are separated by 2.7" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1419 Danzig -1 0 1 14.4 -0 -0
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:03:57.01 -03:09:06.8: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:03:57.01 -03:09:06.8: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461291.8524,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260908.3524 14.35CV 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: 2461242.93295420 21.07.2026 10:23:17.243 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
First image: 2461242.93295420 21.07.2026 10:23:17.243 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Last image: 2461291.85274458 08.09.2026 08:27:47.132 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
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): 5415
Objects passed selection criteria: 5413
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 5245.5
Average stars matched: 5153.75 (98.2509 %)
Memory usage VmPeak: 232680 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 8 03:31:59 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: 2461242.93295420 21.07.2026 10:23:17.243 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
First image: 2461242.93295420 21.07.2026 10:23:17.243 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Last image: 2461291.85274458 08.09.2026 08:27:47.132 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 65
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 18 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): 35351
Objects passed selection criteria: 35260
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 33690
Average stars matched: 32669.5 (96.9709 %)
Memory usage VmPeak: 260408 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 8 03:32:56 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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
SExtractor catalog cache: saved Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.cat to cache
SExtractor catalog cache: saved Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461291.85199922
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits exists and is non-empty
wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits exists and is non-empty
wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits exists and is non-empty
wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (1st reference image)
verification OK: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Image size: 937.5'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: 22:17:09.355 -02:00:05.25 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits (1st new image)
verification OK: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
Image size: 937.0'x624.0' 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: 22:17:09.477 -01:59:55.67 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:09.355 -02:00:05.25
Second-epoch image center 22:17:09.477 -01:59:55.67
Angular distance between the image centers 0.0027 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits (2nd new image)
verification OK: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Image size: 937.0'x624.0' 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: 22:17:06.576 -02:00:31.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:09.355 -02:00:05.25
Second-epoch image center 22:17:06.576 -02:00:31.79
Angular distance between the image centers 0.0137 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 22:17:09.477 -01:59:55.67
Second-epoch second image center 22:17:06.576 -02:00:31.79
Angular distance between the image centers 0.01570 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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits &> /tmp/tmp.msxXR7uDPU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits &> /tmp/tmp.CUWqp4buvi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits &> /tmp/tmp.o6zb2acjPN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits &> /tmp/tmp.wxpzid3Og6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
Found non-empty wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
The reference image (wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits) and catalog (wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat) found
'wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat' -> 'wcsmag.cat'
Read 7776 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4297 to 342.1786 deg, Dec -7.2616 to +3.2651 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 326.4297 to 342.1786 deg, Dec -7.2616 to 3.2651 deg
Loaded 5154 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): 4414 out of 4557 total matches.
Matched with Tycho-2 4557 out of 7776 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.628200
a=0.000000 b=1.000000 c=22.628200
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.08
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.08
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7776 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4297 to 342.1786 deg, Dec -7.2616 to +3.2651 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 326.4297 to 342.1786 deg, Dec -7.2616 to 3.2651 deg
Loaded 5154 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): 4414 out of 4557 total matches.
Matched with Tycho-2 4557 out of 7776 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -> calib.txt_param_ref_wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (aperture=6.2)
Read 7733 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4352 to 342.1813 deg, Dec -7.2521 to +3.2799 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 326.4352 to 342.1813 deg, Dec -7.2521 to 3.2799 deg
Loaded 5154 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): 4402 out of 4552 total matches.
Matched with Tycho-2 4552 out of 7733 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -> calib.txt_param_ref_wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
2.3 pix Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
2.3 pix fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
2.3 pix fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Limiting magnitude estimates:
15.1 mag. Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
15.1 mag. Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
14.8 mag. fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
14.8 mag. fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (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
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.msxXR7uDPU (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_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits' -> 'wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS-calibrated image found: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Checking if the catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS catalog name: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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=420, bad_region=2142, passed=7776
Got 7776 stars (including 5312 good ones) from the SExtractor catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
util/solve_plate_with_UCAC5 got 7776 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4530 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4509 matched stars entering correct_measured_positions(), 4509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4509 matched stars entering correct_measured_positions(), 6065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4529 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4508 matched stars entering correct_measured_positions(), 6065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4508 matched stars entering correct_measured_positions(), 6065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4508 stars left (next iteration limit 4959)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits N_match=4508 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.338 n_q1=1393 n_q2=902 n_q3=1359 n_q4=854 worst_quadrant_to_overall_ratio=1.017
The image catalog is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -region wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.CUWqp4buvi (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_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits' -> 'wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS-calibrated image found: wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Checking if the catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS catalog name: wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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=446, bad_region=2127, passed=7733
Got 7733 stars (including 5260 good ones) from the SExtractor catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat
util/solve_plate_with_UCAC5 got 7733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4539 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 4515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 6014 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4539 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4514 matched stars entering correct_measured_positions(), 6014 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4514 matched stars entering correct_measured_positions(), 6014 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4514 stars left (next iteration limit 4966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits N_match=4514 sigma_overall_arcsec=0.418 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.433 sigma_q3_arcsec=0.430 sigma_q4_arcsec=0.411 n_q1=1390 n_q2=906 n_q3=1375 n_q4=843 worst_quadrant_to_overall_ratio=1.038
The image catalog is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -region wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.o6zb2acjPN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
Checking if the catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
WCS catalog name: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.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=445, bad_region=1622, passed=6588
Got 6588 stars (including 4677 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat
util/solve_plate_with_UCAC5 got 6588 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4243 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4225 matched stars entering correct_measured_positions(), 4226 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4224 matched stars entering correct_measured_positions(), 5318 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4243 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4225 matched stars entering correct_measured_positions(), 5318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4225 matched stars entering correct_measured_positions(), 5318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4225 stars left (next iteration limit 4646)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4225 robust_rms=7.136 arcsec worst_quadrant_rms=8.429 arcsec
SIP_REFIT: SIP order 3 trial: matched=4225 robust_rms=0.398 arcsec worst_quadrant_rms=0.452 arcsec
SIP_REFIT: SIP order 5 trial: matched=4225 robust_rms=0.346 arcsec worst_quadrant_rms=0.368 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4225 robust_rms_before=0.809 arcsec robust_rms_before_corrected=0.368 arcsec robust_rms_after=0.346 arcsec worst_quadrant_rms_before=0.416 worst_quadrant_rms_after=0.368
verification OK: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
verification OK: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.512 -01:59:56.06 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 6588 stars ###
'wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/correct_sextractor_wcs_catalog_usingxy2sky3412360.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.809 -> 0.346 arcsec)
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits N_match=4225 sigma_overall_arcsec=0.375 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.414 sigma_q3_arcsec=0.370 sigma_q4_arcsec=0.386 n_q1=1300 n_q2=894 n_q3=1248 n_q4=783 worst_quadrant_to_overall_ratio=1.105
The image catalog is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits -region wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.wxpzid3Og6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Checking if the catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
WCS catalog name: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.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=415, bad_region=1623, passed=6531
Got 6531 stars (including 4642 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat
util/solve_plate_with_UCAC5 got 6531 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4196 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4174 matched stars entering correct_measured_positions(), 4174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4173 matched stars entering correct_measured_positions(), 5259 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4197 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4175 matched stars entering correct_measured_positions(), 5259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4175 matched stars entering correct_measured_positions(), 5259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4175 stars left (next iteration limit 4590)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4175 robust_rms=7.255 arcsec worst_quadrant_rms=8.378 arcsec
SIP_REFIT: SIP order 3 trial: matched=4175 robust_rms=0.392 arcsec worst_quadrant_rms=0.424 arcsec
SIP_REFIT: SIP order 5 trial: matched=4175 robust_rms=0.341 arcsec worst_quadrant_rms=0.385 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4175 robust_rms_before=0.802 arcsec robust_rms_before_corrected=0.366 arcsec robust_rms_after=0.341 arcsec worst_quadrant_rms_before=0.398 worst_quadrant_rms_after=0.385
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.398 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits N_match=4175 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.348 sigma_q2_arcsec=0.410 sigma_q3_arcsec=0.358 sigma_q4_arcsec=0.376 n_q1=1281 n_q2=888 n_q3=1229 n_q4=777 worst_quadrant_to_overall_ratio=1.055
The image catalog is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits -region wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits to local_wcs_cache/
'wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits' -> 'local_wcs_cache/wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits'
Saving the final (post-refit) wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits to local_wcs_cache/
'wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits' -> 'local_wcs_cache/wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits'
Saving the final (post-refit) wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits to local_wcs_cache/
'wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits' -> 'local_wcs_cache/wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits'
Saving the final (post-refit) wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits to local_wcs_cache/
'wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits' -> 'local_wcs_cache/wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits sigma_overall=0.379 worst_q_ratio=1.017
ref2=Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits sigma_overall=0.418 worst_q_ratio=1.038
new1=fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits sigma_overall=0.375 worst_q_ratio=1.105
new2=fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits sigma_overall=0.389 worst_q_ratio=1.055
reference average sigma_overall=0.3985 worst_q_ratio=1.0275
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013_astrometric_residuals.png (4508 matched stars from wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014_astrometric_residuals.png (4514 matched stars from wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292_astrometric_residuals.png (4225 matched stars from wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293_astrometric_residuals.png (4175 matched stars from wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits'
Saving fully-calibrated image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits'
Preparing the HTML report for the field Aqr-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aqr-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
SExtractor catalog cache: saved Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.cat to cache
SExtractor catalog cache: saved Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Creating symlink local_wcs_cache/wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits exists and is non-empty
wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits exists and is non-empty
wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits exists and is non-empty
wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (1st reference image)
verification OK: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Image size: 937.5'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: 22:17:09.355 -02:00:05.25 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits (1st new image)
verification OK: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.512 -01:59:56.06 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:09.355 -02:00:05.25
Second-epoch image center 22:17:09.512 -01:59:56.06
Angular distance between the image centers 0.0026 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits (2nd new image)
verification OK: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Image size: 937.0'x624.0' 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: 22:17:06.576 -02:00:31.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:09.355 -02:00:05.25
Second-epoch image center 22:17:06.576 -02:00:31.79
Angular distance between the image centers 0.0137 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 22:17:09.512 -01:59:56.06
Second-epoch second image center 22:17:06.576 -02:00:31.79
Angular distance between the image centers 0.01575 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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits &> /tmp/tmp.7sRoa16Y2r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits &> /tmp/tmp.jw7GOKCZFJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits &> /tmp/tmp.DDMv2OpluZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits &> /tmp/tmp.ozKuj6gvoZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
Found non-empty wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
The reference image (wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits) and catalog (wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat) found
'wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat' -> 'wcsmag.cat'
Read 46863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4298 to 342.1802 deg, Dec -7.2660 to +3.2673 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 326.4298 to 342.1802 deg, Dec -7.2660 to 3.2673 deg
Loaded 5156 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): 4240 out of 4650 total matches.
Matched with Tycho-2 4650 out of 46863 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.491650
a=0.000000 b=1.000000 c=22.491650
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 46863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4298 to 342.1802 deg, Dec -7.2660 to +3.2673 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 326.4298 to 342.1802 deg, Dec -7.2660 to 3.2673 deg
Loaded 5156 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): 4240 out of 4650 total matches.
Matched with Tycho-2 4650 out of 46863 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -> calib.txt_param_ref_wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (aperture=4.7)
Read 47307 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.4340 to 342.1839 deg, Dec -7.2541 to +3.2809 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 326.4340 to 342.1839 deg, Dec -7.2541 to 3.2809 deg
Loaded 5159 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): 4244 out of 4656 total matches.
Matched with Tycho-2 4656 out of 47307 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -> calib.txt_param_ref_wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 46 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
2.1 pix Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
2.1 pix fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
2.1 pix fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Limiting magnitude estimates:
15.3 mag. Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
15.2 mag. Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
15.0 mag. fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
15.0 mag. fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (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.7sRoa16Y2r (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_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits' -> 'wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS-calibrated image found: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Checking if the catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS catalog name: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.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=19, blended=2071, bad_region=10220, passed=46844
Got 46844 stars (including 35017 good ones) from the SExtractor catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
util/solve_plate_with_UCAC5 got 46844 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4525 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 4507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4525 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4507 stars left (next iteration limit 4957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits N_match=4507 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.356 sigma_q2_arcsec=0.371 sigma_q3_arcsec=0.366 sigma_q4_arcsec=0.325 n_q1=1375 n_q2=933 n_q3=1339 n_q4=860 worst_quadrant_to_overall_ratio=1.028
The image catalog is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -region wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.jw7GOKCZFJ (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_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits' -> 'wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.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-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS-calibrated image found: wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Checking if the catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS catalog name: wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2102, bad_region=10366, passed=47292
Got 47292 stars (including 35288 good ones) from the SExtractor catalog wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat
util/solve_plate_with_UCAC5 got 47292 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4526 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 4507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4526 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 39363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4507 stars left (next iteration limit 4957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits N_match=4507 sigma_overall_arcsec=0.401 sigma_q1_arcsec=0.390 sigma_q2_arcsec=0.419 sigma_q3_arcsec=0.413 sigma_q4_arcsec=0.390 n_q1=1375 n_q2=926 n_q3=1338 n_q4=868 worst_quadrant_to_overall_ratio=1.044
The image catalog is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -region wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.DDMv2OpluZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
Checking if the catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
WCS catalog name: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.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=2223, bad_region=6561, passed=37580
Got 37580 stars (including 29863 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat
util/solve_plate_with_UCAC5 got 37580 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4519 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4502 matched stars entering correct_measured_positions(), 4502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4502 matched stars entering correct_measured_positions(), 32638 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4518 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4502 matched stars entering correct_measured_positions(), 32638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4502 matched stars entering correct_measured_positions(), 32638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4502 stars left (next iteration limit 4952)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4502 robust_rms=6.705 arcsec worst_quadrant_rms=9.550 arcsec
SIP_REFIT: SIP order 3 trial: matched=4502 robust_rms=0.394 arcsec worst_quadrant_rms=0.448 arcsec
SIP_REFIT: SIP order 5 trial: matched=4502 robust_rms=0.341 arcsec worst_quadrant_rms=0.357 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4502 robust_rms_before=0.344 arcsec robust_rms_before_corrected=0.355 arcsec robust_rms_after=0.341 arcsec worst_quadrant_rms_before=0.362 worst_quadrant_rms_after=0.357
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.362 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits N_match=4502 sigma_overall_arcsec=0.373 sigma_q1_arcsec=0.335 sigma_q2_arcsec=0.413 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.393 n_q1=1444 n_q2=886 n_q3=1386 n_q4=786 worst_quadrant_to_overall_ratio=1.105
The image catalog is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits -region wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ozKuj6gvoZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Checking if the catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
WCS catalog name: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.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=2208, bad_region=6576, passed=37615
Got 37615 stars (including 29893 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat
util/solve_plate_with_UCAC5 got 37615 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4511 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4491 matched stars entering correct_measured_positions(), 4491 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4491 matched stars entering correct_measured_positions(), 32654 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4511 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4492 matched stars entering correct_measured_positions(), 32654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4492 matched stars entering correct_measured_positions(), 32654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4492 stars left (next iteration limit 4940)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4492 robust_rms=6.728 arcsec worst_quadrant_rms=9.461 arcsec
SIP_REFIT: SIP order 3 trial: matched=4492 robust_rms=0.390 arcsec worst_quadrant_rms=0.425 arcsec
SIP_REFIT: SIP order 5 trial: matched=4492 robust_rms=0.339 arcsec worst_quadrant_rms=0.383 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4492 robust_rms_before=0.798 arcsec robust_rms_before_corrected=0.356 arcsec robust_rms_after=0.339 arcsec worst_quadrant_rms_before=0.399 worst_quadrant_rms_after=0.383
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.399 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits N_match=4492 sigma_overall_arcsec=0.375 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.419 sigma_q3_arcsec=0.350 sigma_q4_arcsec=0.372 n_q1=1442 n_q2=889 n_q3=1379 n_q4=782 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits -region wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-26-42_20.00sec_-0.00C_LIGHT_0292.fits
Saving fully-calibrated image wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-08_CI_Aqr-02-Q2b1x1_032837_TTUQ2b1x1_3234048_qG2c923n/wcs_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293.fits
Preparing the HTML report for the field Aqr-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:27:30.24 +02:09:31.8: 14.52 +/- 0.10 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:30:46.28 -03:04:17.2: 14.28 +/- 0.09 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:36:00.10 -01:43:23.5: 15.05 +/- 0.20 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:28:03.95 -05:56:44.7: 12.99 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:32:34.70 +01:33:44.7: 12.91 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:37:10.58 -01:29:45.8: 13.94 +/- 0.07 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:05:35.60 -02:53:54.7: 14.10 +/- 0.07 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:39:00.40 +01:00:49.2: 13.76 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:32:36.67 +00:06:57.0: 13.39 +/- 0.04 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:37:19.23 -00:08:50.8: 13.75 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:27:30.24 +02:09:31.8: 14.65 +/- 0.12 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:28:03.95 -05:56:44.7: 13.02 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:30:46.28 -03:04:17.2: 14.48 +/- 0.11 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:36:00.10 -01:43:23.5: 15.19 +/- 0.21 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:32:34.70 +01:33:44.7: 12.90 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:32:36.67 +00:06:57.0: 13.48 +/- 0.04 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:37:10.58 -01:29:45.8: 14.03 +/- 0.07 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:05:35.60 -02:53:54.7: 14.19 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.07
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry reference-image weighted average: 14.57 +/- 0.08
Forced photometry filter REJECTED candidate at 22:30:46.28 -03:04:17.2: ref_mag=14.36 +/- 0.07 new_mean_mag=14.4474 delta=-0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:28:03.95 -05:56:44.7: ref_mag=13.01 +/- 0.02 new_mean_mag=12.9741 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 15.12 +/- 0.14
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry reference-image weighted average: 13.98 +/- 0.05
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter REJECTED candidate at 22:27:30.24 +02:09:31.8: ref_mag=14.57 +/- 0.08 new_mean_mag=14.8144 delta=-0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:32:36.67 +00:06:57.0: ref_mag=13.43 +/- 0.03 new_mean_mag=13.5953 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 14.14 +/- 0.05
Forced photometry filter REJECTED candidate at 22:36:00.10 -01:43:23.5: ref_mag=15.12 +/- 0.14 new_mean_mag=14.7881 delta=0.33 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:37:10.58 -01:29:45.8: ref_mag=13.98 +/- 0.05 new_mean_mag=14.1240 delta=-0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:32:34.70 +01:33:44.7: ref_mag=12.90 +/- 0.02 new_mean_mag=12.9362 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:05:35.60 -02:53:54.7: ref_mag=14.14 +/- 0.05 new_mean_mag=14.4407 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:37:19.23 -00:08:50.8: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter REJECTED candidate at 22:37:19.23 -00:08:50.8: ref_mag=13.75 +/- 0.04 new_mean_mag=13.7852 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:39:00.40 +01:00:49.2: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter REJECTED candidate at 22:39:00.40 +01:00:49.2: ref_mag=13.68 +/- 0.04 new_mean_mag=13.6369 delta=0.05 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:27:05.88 -03:25:57.1: 13.68 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:26:18.58 -05:10:12.5: 13.73 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:36:50.11 -00:05:48.4: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:44:31.92 -02:17:41.8: 13.94 +/- 0.08 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:40:41.99 -03:39:08.2: 14.15 +/- 0.09 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:22:02.51 -01:55:03.8: 13.89 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:31:48.00 -04:13:08.8: 13.91 +/- 0.07 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:40:13.14 +00:57:53.5: 15.09 +/- 0.21 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:39:31.37 -00:15:16.8: 14.80 +/- 0.15 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:26:18.58 -05:10:12.5: 13.63 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.04
Forced photometry filter REJECTED candidate at 22:26:18.58 -05:10:12.5: ref_mag=13.67 +/- 0.04 new_mean_mag=13.7698 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:27:05.88 -03:25:57.1: 13.65 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:36:50.11 -00:05:48.4: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:42:47.17 +01:29:11.8: 14.96 +/- 0.20 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:44:31.92 -02:17:41.8: 14.05 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Forced photometry filter REJECTED candidate at 22:27:05.88 -03:25:57.1: ref_mag=13.66 +/- 0.04 new_mean_mag=13.8024 delta=-0.14 (need > 0.90)
Forced photometry reference-image weighted average: 14.00 +/- 0.06
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:40:41.99 -03:39:08.2: 14.16 +/- 0.09 detection
Forced photometry filter REJECTED candidate at 22:44:31.92 -02:17:41.8: ref_mag=14.00 +/- 0.06 new_mean_mag=14.2003 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:22:02.51 -01:55:03.8: 14.05 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.07
Forced photometry filter REJECTED candidate at 22:40:41.99 -03:39:08.2: ref_mag=14.15 +/- 0.07 new_mean_mag=14.1392 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Forced photometry filter REJECTED candidate at 22:22:02.51 -01:55:03.8: ref_mag=13.96 +/- 0.05 new_mean_mag=14.0161 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:31:48.00 -04:13:08.8: 13.89 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Forced photometry filter REJECTED candidate at 22:31:48.00 -04:13:08.8: ref_mag=13.90 +/- 0.05 new_mean_mag=13.9400 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:40:13.14 +00:57:53.5: 14.92 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.13
Forced photometry filter REJECTED candidate at 22:40:13.14 +00:57:53.5: ref_mag=14.99 +/- 0.13 new_mean_mag=14.6071 delta=0.38 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:39:31.37 -00:15:16.8: 14.75 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.11
Forced photometry filter REJECTED candidate at 22:39:31.37 -00:15:16.8: ref_mag=14.78 +/- 0.11 new_mean_mag=14.4339 delta=0.34 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:42:47.17 +01:29:11.8: 14.93 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.14
Forced photometry filter REJECTED candidate at 22:42:47.17 +01:29:11.8: ref_mag=14.94 +/- 0.14 new_mean_mag=14.7720 delta=0.17 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:43:14.46 -05:33:33.8: 15.14 +/- 0.25 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:12:26.18 +02:05:08.1: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:41:58.67 -05:59:56.8: 14.74 +/- 0.18 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:41:10.63 -05:09:07.9: 14.99 +/- 0.21 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:40:22.44 -01:54:24.3: 14.84 +/- 0.17 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:42:06.31 -05:10:55.4: 15.01 +/- 0.22 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:42:54.86 -03:38:05.3: 14.99 +/- 0.21 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:36:12.42 +01:44:43.3: 14.87 +/- 0.16 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:43:14.46 -05:33:33.8: 15.36 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.19
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:12:26.18 +02:05:08.1: 15.95 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 22:43:14.46 -05:33:33.8: ref_mag=15.23 +/- 0.19 new_mean_mag=14.7523 delta=0.47 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:41:58.67 -05:59:56.8: 14.72 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.73 +/- 0.12
Forced photometry filter REJECTED candidate at 22:41:58.67 -05:59:56.8: ref_mag=14.73 +/- 0.12 new_mean_mag=14.5892 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:41:10.63 -05:09:07.9: 14.84 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.13
Forced photometry filter REJECTED candidate at 22:41:10.63 -05:09:07.9: ref_mag=14.90 +/- 0.13 new_mean_mag=14.6525 delta=0.25 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:42:06.31 -05:10:55.4: 14.66 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.13
Forced photometry filter REJECTED candidate at 22:42:06.31 -05:10:55.4: ref_mag=14.78 +/- 0.13 new_mean_mag=14.6651 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:42:54.86 -03:38:05.3: 14.89 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.14
Forced photometry filter REJECTED candidate at 22:42:54.86 -03:38:05.3: ref_mag=14.94 +/- 0.14 new_mean_mag=14.6931 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:40:22.44 -01:54:24.3: 14.60 +/- 0.14 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:36:05.34 +01:26:05.5: 14.97 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.69 +/- 0.11
Forced photometry filter REJECTED candidate at 22:40:22.44 -01:54:24.3: ref_mag=14.69 +/- 0.11 new_mean_mag=14.5357 delta=0.16 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:36:12.42 +01:44:43.3: 15.02 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.13
Forced photometry filter REJECTED candidate at 22:36:12.42 +01:44:43.3: ref_mag=14.92 +/- 0.13 new_mean_mag=14.5998 delta=0.32 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:36:05.34 +01:26:05.5: 14.85 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.12
Forced photometry filter REJECTED candidate at 22:36:05.34 +01:26:05.5: ref_mag=14.90 +/- 0.12 new_mean_mag=14.6984 delta=0.21 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:44:11.59 -01:52:14.3: 15.15 +/- 0.25 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:08:45.64 -04:57:24.7: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:44:33.18 -02:10:20.9: 15.02 +/- 0.21 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:30:33.02 -00:46:01.1: 15.08 +/- 0.20 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:44:03.22 -02:29:58.2: 14.36 +/- 0.12 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:41:26.29 -01:49:07.6: 15.02 +/- 0.21 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:44:11.59 -01:52:14.3: 14.88 +/- 0.19 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:44:33.18 -02:10:20.9: 15.06 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.15
Forced photometry filter REJECTED candidate at 22:44:11.59 -01:52:14.3: ref_mag=14.97 +/- 0.15 new_mean_mag=14.8260 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 15.04 +/- 0.15
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:08:45.64 -04:57:24.7: 15.83 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 22:44:33.18 -02:10:20.9: ref_mag=15.04 +/- 0.15 new_mean_mag=14.7820 delta=0.26 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:03:57.01 -03:09:06.8: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:30:33.02 -00:46:01.1: 14.91 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.13
Forced photometry filter REJECTED candidate at 22:30:33.02 -00:46:01.1: ref_mag=14.98 +/- 0.13 new_mean_mag=14.7252 delta=0.26 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:44:03.22 -02:29:58.2: 14.42 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.09
Forced photometry filter REJECTED candidate at 22:44:03.22 -02:29:58.2: ref_mag=14.39 +/- 0.09 new_mean_mag=14.5140 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:41:26.29 -01:49:07.6: 14.93 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.14
Forced photometry filter REJECTED candidate at 22:41:26.29 -01:49:07.6: ref_mag=14.97 +/- 0.14 new_mean_mag=14.7571 delta=0.21 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:37:48.39 -04:18:06.6: 14.83 +/- 0.16 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:03:57.01 -03:09:06.8: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:37:48.39 -04:18:06.6: 14.90 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.12
Forced photometry filter REJECTED candidate at 22:37:48.39 -04:18:06.6: ref_mag=14.86 +/- 0.12 new_mean_mag=14.7158 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:10:29.83 -02:51:33.6: 14.64 +/- 0.13 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:24:37.68 -05:24:12.0: 15.00 +/- 0.18 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:34:07.23 -01:16:54.4: 15.15 +/- 0.20 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:33:24.87 -03:01:01.5: 14.87 +/- 0.15 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:24:26.18 -02:19:24.0: 15.67 +/- 0.30 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:10:29.83 -02:51:33.6: 14.61 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.09
Forced photometry filter REJECTED candidate at 22:10:29.83 -02:51:33.6: ref_mag=14.63 +/- 0.09 new_mean_mag=14.6601 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:24:37.68 -05:24:12.0: 15.45 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.14 +/- 0.15
Forced photometry filter REJECTED candidate at 22:24:37.68 -05:24:12.0: ref_mag=15.14 +/- 0.15 new_mean_mag=14.7274 delta=0.41 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:34:07.23 -01:16:54.4: 15.16 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.14
Forced photometry filter REJECTED candidate at 22:34:07.23 -01:16:54.4: ref_mag=15.15 +/- 0.14 new_mean_mag=14.8160 delta=0.34 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:33:24.87 -03:01:01.5: 15.15 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.12
Forced photometry filter REJECTED candidate at 22:33:24.87 -03:01:01.5: ref_mag=14.98 +/- 0.12 new_mean_mag=14.8477 delta=0.13 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:24:26.18 -02:19:24.0: 15.03 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.15
Forced photometry filter REJECTED candidate at 22:24:26.18 -02:19:24.0: ref_mag=15.19 +/- 0.15 new_mean_mag=14.8262 delta=0.36 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:27:04.20 -02:01:04.8: 15.17 +/- 0.20 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:27:04.20 -02:01:04.8: 15.19 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.18 +/- 0.14
Forced photometry filter REJECTED candidate at 22:27:04.20 -02:01:04.8: ref_mag=15.18 +/- 0.14 new_mean_mag=14.8762 delta=0.31 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:19:07.04 -05:53:57.3: 15.02 +/- 0.18 detection
Forced photometry on wcs_Aqr-02-Q2b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:19:07.04 -05:53:57.3: 15.21 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.14
Forced photometry filter REJECTED candidate at 22:19:07.04 -05:53:57.3: ref_mag=15.10 +/- 0.14 new_mean_mag=14.7832 delta=0.31 (need > 0.90)
Adding exclusion_list_local.txt__out53125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53208.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53047_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53047_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53053_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53053_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53054_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53054_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53057_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53057_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53061_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53061_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53076_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53076_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53077_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53077_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53093_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53093_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53095_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53095_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53100_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53100_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53103_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53103_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53108_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53108_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53111_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53111_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53113_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53113_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
**** FOUND 22:12:42.88 -04:41:43.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53114_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53114_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53117_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53117_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53120_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53120_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53125_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
Preparing report for the candidate 53125_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53126_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53126_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53136_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53136_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53152_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53152_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53158_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53158_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53160_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53160_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53161_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
Preparing report for the candidate 53161_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53162_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53162_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53164_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53164_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53167_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53167_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53168_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53168_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53172_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53172_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53177_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53177_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53182_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53182_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53188_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
Preparing report for the candidate 53188_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53191_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53191_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53197_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53197_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53200_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53200_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53207_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53207_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53208_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
Preparing report for the candidate 53208_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53212_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53212_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53215_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53215_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53218_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53218_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53219_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53219_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53224_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53224_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53231_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53231_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53279_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53279_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53299_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 53299_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17171_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293
The candidate 17171_fd_Aqr-02-Q2b1x1_2026-09-08_03-27-47_20.00sec_-0.00C_LIGHT_0293 did not pass the final checks