This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb
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 01.2591 2461284.7591 13.97 22:41:37.42 +00:44:05.2
69.37050 -48.16652 galactic Aqr Second-epoch detections are separated by 1.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1023 Thomana 0 0 0 14.3 -0 -0
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:41:37.42 +00:44:05.2: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:41:37.42 +00:44:05.2: 15.66 +/- 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,2461284.7591,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260901.2591 13.97CV 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 01.2591 2461284.7591 14.31 22:10:19.16 -02:17:28.0
58.71197 -44.15934 galactic Aqr Second-epoch detections are separated by 2.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1419 Danzig -0 -1 1 14.3 -0 -0
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:10:19.16 -02:17:28.0: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:10:19.16 -02:17:28.0: 15.92 +/- 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,2461284.7591,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260901.2591 14.31CV 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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Last image: 2461284.75936022 01.09.2026 06:13:18.723 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.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.: -7.58
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: 3 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): 7480
Objects passed selection criteria: 7465
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 6444.25
Average stars matched: 6291.5 (97.6297 %)
Memory usage VmPeak: 233668 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 1 01:18:59 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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Last image: 2461284.75936022 01.09.2026 06:13:18.723 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 43937
Objects passed selection criteria: 43814
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 37094.5
Average stars matched: 35829.8 (96.5905 %)
Memory usage VmPeak: 266080 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 1 01:19:59 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
SExtractor catalog cache: saved Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.cat to cache
SExtractor catalog cache: saved Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.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: 2461284.75881189
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits exists and is non-empty
wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits exists and is non-empty
wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits exists and is non-empty
wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (1st reference image)
verification OK: wcs_Aqr-02-Q1b1x1_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-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits (1st new image)
verification OK: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
Image size: 940.8'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 22:16:58.256 -02:00:45.19 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 22:16:58.256 -02:00:45.19
Angular distance between the image centers 0.0475 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits (2nd new image)
verification OK: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Image size: 940.8'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 22:16:59.471 -02:01:24.57 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 22:16:59.471 -02:01:24.57
Angular distance between the image centers 0.0467 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 22:16:58.256 -02:00:45.19
Second-epoch second image center 22:16:59.471 -02:01:24.57
Angular distance between the image centers 0.01205 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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits &> /tmp/tmp.q0CVbMFrop
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits &> /tmp/tmp.t5YuHafwvR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits &> /tmp/tmp.IbINwNDh4X
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits &> /tmp/tmp.hYlWEDWC8s
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
Found non-empty wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
The reference image (wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits) and catalog (wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat) found
'wcs_Aqr-02-Q1b1x1_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 22.640350
a=0.000000 b=1.000000 c=22.640350
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.06
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.06
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -> calib.txt_param_ref_wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (aperture=6.4)
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -> calib.txt_param_ref_wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
2.3 pix Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
3.0 pix fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
3.0 pix fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Limiting magnitude estimates:
15.1 mag. Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
15.1 mag. Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
14.3 mag. fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
14.3 mag. fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.q0CVbMFrop (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits' -> 'wcs_Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS-calibrated image found: wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Checking if the catalog wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS catalog name: wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=420, bad_region=0, passed=7776
Got 7776 stars (including 7348 good ones) from the SExtractor catalog wcs_Aqr-02-Q1b1x1_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 4564 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4544 matched stars entering correct_measured_positions(), 4544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4544 matched stars entering correct_measured_positions(), 7776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4565 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4545 matched stars entering correct_measured_positions(), 7776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4545 matched stars entering correct_measured_positions(), 7776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4545 stars left (next iteration limit 4998)
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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits N_match=4545 sigma_overall_arcsec=0.432 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.484 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.442 n_q1=1032 n_q2=1269 n_q3=1017 n_q4=1227 worst_quadrant_to_overall_ratio=1.120
The image catalog is written to wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -region wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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.t5YuHafwvR (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits' -> 'wcs_Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS-calibrated image found: wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Checking if the catalog wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS catalog name: wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=446, bad_region=0, passed=7733
Got 7733 stars (including 7277 good ones) from the SExtractor catalog wcs_Aqr-02-Q1b1x1_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 4564 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4543 matched stars entering correct_measured_positions(), 4543 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4543 matched stars entering correct_measured_positions(), 7733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4562 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4542 matched stars entering correct_measured_positions(), 7733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4542 matched stars entering correct_measured_positions(), 7733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4542 stars left (next iteration limit 4997)
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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits N_match=4542 sigma_overall_arcsec=0.467 sigma_q1_arcsec=0.393 sigma_q2_arcsec=0.501 sigma_q3_arcsec=0.429 sigma_q4_arcsec=0.482 n_q1=1033 n_q2=1270 n_q3=1019 n_q4=1220 worst_quadrant_to_overall_ratio=1.073
The image catalog is written to wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -region wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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.IbINwNDh4X (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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
Checking if the catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
WCS catalog name: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=273, bad_region=0, passed=5161
Got 5161 stars (including 4882 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat
util/solve_plate_with_UCAC5 got 5161 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 4453 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4429 matched stars entering correct_measured_positions(), 4429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4429 matched stars entering correct_measured_positions(), 5161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 4454 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4429 matched stars entering correct_measured_positions(), 5161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4429 matched stars entering correct_measured_positions(), 5161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4429 stars left (next iteration limit 4871)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4429 robust_rms=10.630 arcsec worst_quadrant_rms=15.790 arcsec
SIP_REFIT: SIP order 3 trial: matched=4429 robust_rms=0.425 arcsec worst_quadrant_rms=0.436 arcsec
SIP_REFIT: SIP order 5 trial: matched=4429 robust_rms=0.321 arcsec worst_quadrant_rms=0.377 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4429 robust_rms_before=0.880 arcsec robust_rms_before_corrected=0.338 arcsec robust_rms_after=0.321 arcsec worst_quadrant_rms_before=0.426 worst_quadrant_rms_after=0.377
verification OK: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
verification OK: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:58.278 -02:00:46.02 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5161 stars ###
'wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/correct_sextractor_wcs_catalog_usingxy2sky480241.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.880 -> 0.321 arcsec)
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits N_match=4429 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.382 sigma_q2_arcsec=0.366 sigma_q3_arcsec=0.298 sigma_q4_arcsec=0.294 n_q1=1228 n_q2=964 n_q3=1268 n_q4=969 worst_quadrant_to_overall_ratio=1.162
The image catalog is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits -region wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.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.hYlWEDWC8s (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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Checking if the catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
WCS catalog name: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=281, bad_region=0, passed=5260
Got 5260 stars (including 4977 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat
util/solve_plate_with_UCAC5 got 5260 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 4533 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4508 matched stars entering correct_measured_positions(), 4508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4508 matched stars entering correct_measured_positions(), 5260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 4535 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4510 matched stars entering correct_measured_positions(), 5260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4510 matched stars entering correct_measured_positions(), 5260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4510 stars left (next iteration limit 4958)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4510 robust_rms=10.731 arcsec worst_quadrant_rms=15.302 arcsec
SIP_REFIT: SIP order 3 trial: matched=4510 robust_rms=0.403 arcsec worst_quadrant_rms=0.417 arcsec
SIP_REFIT: SIP order 5 trial: matched=4510 robust_rms=0.306 arcsec worst_quadrant_rms=0.357 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4510 robust_rms_before=0.872 arcsec robust_rms_before_corrected=0.320 arcsec robust_rms_after=0.306 arcsec worst_quadrant_rms_before=0.399 worst_quadrant_rms_after=0.357
verification OK: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
verification OK: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:59.492 -02:01:25.37 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5260 stars ###
'wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/correct_sextractor_wcs_catalog_usingxy2sky480211.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.872 -> 0.306 arcsec)
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits N_match=4510 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.362 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.278 sigma_q4_arcsec=0.306 n_q1=1251 n_q2=983 n_q3=1293 n_q4=983 worst_quadrant_to_overall_ratio=1.134
The image catalog is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits -region wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits to local_wcs_cache/
'wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits' -> 'local_wcs_cache/wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits'
Saving the final (post-refit) wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits to local_wcs_cache/
'wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits' -> 'local_wcs_cache/wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits'
Saving the final (post-refit) wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits to local_wcs_cache/
'wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits' -> 'local_wcs_cache/wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits'
Saving the final (post-refit) wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits to local_wcs_cache/
'wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits' -> 'local_wcs_cache/wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits sigma_overall=0.432 worst_q_ratio=1.120
ref2=Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits sigma_overall=0.467 worst_q_ratio=1.073
new1=fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits sigma_overall=0.329 worst_q_ratio=1.162
new2=fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits sigma_overall=0.324 worst_q_ratio=1.134
reference average sigma_overall=0.4495 worst_q_ratio=1.0965
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013_astrometric_residuals.png (4545 matched stars from wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014_astrometric_residuals.png (4542 matched stars from wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240_astrometric_residuals.png (4429 matched stars from wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241_astrometric_residuals.png (4510 matched stars from wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits'
Saving fully-calibrated image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits'
Preparing the HTML report for the field Aqr-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:36:10.55 +00:09:50.9: 10.89 +/- 0.00 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:36:10.55 +00:09:50.9: 10.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.90 +/- 0.00
Forced photometry filter REJECTED candidate at 22:36:10.55 +00:09:50.9: ref_mag=10.90 +/- 0.00 new_mean_mag=11.2624 delta=-0.36 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20400_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 20400_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Aqr-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
SExtractor catalog cache: saved Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.cat to cache
SExtractor catalog cache: saved Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Creating symlink local_wcs_cache/wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits exists and is non-empty
wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits exists and is non-empty
wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits exists and is non-empty
wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (1st reference image)
verification OK: wcs_Aqr-02-Q1b1x1_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-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits (1st new image)
verification OK: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:58.278 -02:00:46.02 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 22:16:58.278 -02:00:46.02
Angular distance between the image centers 0.0475 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits (2nd new image)
verification OK: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:16:59.492 -02:01:25.37 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 22:16:59.492 -02:01:25.37
Angular distance between the image centers 0.0467 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 22:16:58.278 -02:00:46.02
Second-epoch second image center 22:16:59.492 -02:01:25.37
Angular distance between the image centers 0.01204 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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits &> /tmp/tmp.lXBvLKktbC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits &> /tmp/tmp.My5LNj3A30
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits &> /tmp/tmp.bLzc3YSuzQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits &> /tmp/tmp.UNC87brHHc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
Found non-empty wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits and wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
The reference image (wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits) and catalog (wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat) found
'wcs_Aqr-02-Q1b1x1_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 22.515400
a=0.000000 b=1.000000 c=22.515400
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -> calib.txt_param_ref_wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits (aperture=4.9)
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Forced-photometry filter: calibrated wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -> calib.txt_param_ref_wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 22 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
2.1 pix Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
2.8 pix fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
2.8 pix fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Limiting magnitude estimates:
15.2 mag. Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
15.2 mag. Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
14.4 mag. fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
14.4 mag. fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.8 (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.lXBvLKktbC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits' -> 'wcs_Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS-calibrated image found: wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
Checking if the catalog wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat corresponding to the image wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits
WCS catalog name: wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=2071, bad_region=0, passed=46835
Got 46835 stars (including 44699 good ones) from the SExtractor catalog wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits.wcscat
util/solve_plate_with_UCAC5 got 46835 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 4552 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4538 matched stars entering correct_measured_positions(), 4538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4538 matched stars entering correct_measured_positions(), 46835 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 4553 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4538 matched stars entering correct_measured_positions(), 46835 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4538 matched stars entering correct_measured_positions(), 46835 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4538 stars left (next iteration limit 4991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits N_match=4538 sigma_overall_arcsec=0.418 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.480 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.422 n_q1=1039 n_q2=1281 n_q3=999 n_q4=1219 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits -region wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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.My5LNj3A30 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits' -> 'wcs_Aqr-02-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS_IMAGE_NAME=wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS-calibrated image found: wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
Checking if the catalog wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits alredy exist and is non-empty...
Catalog wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat corresponding to the image wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits
WCS catalog name: wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=2102, bad_region=1, passed=47281
Got 47281 stars (including 45120 good ones) from the SExtractor catalog wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits.wcscat
util/solve_plate_with_UCAC5 got 47281 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 4553 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4539 matched stars entering correct_measured_positions(), 4539 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4539 matched stars entering correct_measured_positions(), 47281 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4552 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4539 matched stars entering correct_measured_positions(), 47281 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4539 matched stars entering correct_measured_positions(), 47281 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4539 stars left (next iteration limit 4992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits N_match=4539 sigma_overall_arcsec=0.457 sigma_q1_arcsec=0.397 sigma_q2_arcsec=0.500 sigma_q3_arcsec=0.424 sigma_q4_arcsec=0.480 n_q1=1033 n_q2=1281 n_q3=989 n_q4=1236 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits -region wcs_Aqr-02-Q1b1x1_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-Q1b1x1_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.bLzc3YSuzQ (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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
Checking if the catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
WCS catalog name: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=908, bad_region=3, passed=27646
Got 27646 stars (including 26698 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat
util/solve_plate_with_UCAC5 got 27646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4560 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4542 matched stars entering correct_measured_positions(), 4542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4542 matched stars entering correct_measured_positions(), 27646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4561 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4541 matched stars entering correct_measured_positions(), 27646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4541 matched stars entering correct_measured_positions(), 27646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4541 stars left (next iteration limit 4996)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.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=4541 robust_rms=10.190 arcsec worst_quadrant_rms=15.018 arcsec
SIP_REFIT: SIP order 3 trial: matched=4541 robust_rms=0.416 arcsec worst_quadrant_rms=0.431 arcsec
SIP_REFIT: SIP order 5 trial: matched=4541 robust_rms=0.315 arcsec worst_quadrant_rms=0.366 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4541 robust_rms_before=0.317 arcsec robust_rms_before_corrected=0.312 arcsec robust_rms_after=0.315 arcsec worst_quadrant_rms_before=0.361 worst_quadrant_rms_after=0.366
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.361 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits N_match=4541 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.373 sigma_q2_arcsec=0.346 sigma_q3_arcsec=0.278 sigma_q4_arcsec=0.268 n_q1=1192 n_q2=964 n_q3=1314 n_q4=1071 worst_quadrant_to_overall_ratio=1.189
The image catalog is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits -region wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.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.UNC87brHHc (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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
WCS-calibrated image found: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Checking if the catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat corresponding to the image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
WCS catalog name: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=909, bad_region=4, passed=27656
Got 27656 stars (including 26710 good ones) from the SExtractor catalog wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat
util/solve_plate_with_UCAC5 got 27656 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4558 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4539 matched stars entering correct_measured_positions(), 4539 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4539 matched stars entering correct_measured_positions(), 27656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4558 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4539 matched stars entering correct_measured_positions(), 27656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4539 matched stars entering correct_measured_positions(), 27656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4539 stars left (next iteration limit 4992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.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=4539 robust_rms=10.209 arcsec worst_quadrant_rms=15.258 arcsec
SIP_REFIT: SIP order 3 trial: matched=4539 robust_rms=0.397 arcsec worst_quadrant_rms=0.398 arcsec
SIP_REFIT: SIP order 5 trial: matched=4539 robust_rms=0.302 arcsec worst_quadrant_rms=0.348 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4539 robust_rms_before=0.302 arcsec robust_rms_before_corrected=0.304 arcsec robust_rms_after=0.302 arcsec worst_quadrant_rms_before=0.344 worst_quadrant_rms_after=0.348
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.344 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits N_match=4539 sigma_overall_arcsec=0.307 sigma_q1_arcsec=0.351 sigma_q2_arcsec=0.321 sigma_q3_arcsec=0.272 sigma_q4_arcsec=0.275 n_q1=1191 n_q2=974 n_q3=1318 n_q4=1056 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits -region wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.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-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-12-31_20.00sec_0.00C_LIGHTs_0240.fits
Saving fully-calibrated image wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.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_2026-09-01_CI_Aqr-02-Q1b1x1_011358_TTUQ1b1x1_194816_S0g6NEFb/wcs_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241.fits
Preparing the HTML report for the field Aqr-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 21:47:12.20 -03:24:39.7: 12.99 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 21:49:05.71 +03:09:11.6: 13.33 +/- 0.04 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 21:46:43.38 -02:12:58.0: 12.14 +/- 0.02 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:32:34.70 +01:33:44.9: 12.91 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 21:47:41.28 -04:05:24.0: 12.84 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 21:58:39.34 +03:05:33.1: 13.77 +/- 0.05 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 21:48:45.53 -03:21:50.4: 12.83 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:28:03.89 -05:56:44.7: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 21:46:45.73 +00:44:29.4: 13.41 +/- 0.05 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 21:58:39.34 +03:05:33.1: 13.76 +/- 0.05 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 21:47:41.28 -04:05:24.0: 12.75 +/- 0.02 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:32:34.70 +01:33:44.9: 12.90 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 21:48:45.53 -03:21:50.4: 12.86 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:28:03.89 -05:56:44.7: 13.01 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 21:46:43.38 -02:12:58.0: 12.12 +/- 0.02 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 21:47:12.20 -03:24:39.7: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 21:49:05.71 +03:09:11.6: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter REJECTED candidate at 21:47:41.28 -04:05:24.0: ref_mag=12.79 +/- 0.02 new_mean_mag=12.8265 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:58:39.34 +03:05:33.1: ref_mag=13.76 +/- 0.04 new_mean_mag=13.6748 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:48:45.53 -03:21:50.4: ref_mag=12.85 +/- 0.02 new_mean_mag=12.7487 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:32:34.70 +01:33:44.9: ref_mag=12.90 +/- 0.02 new_mean_mag=12.9391 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:28:03.89 -05:56:44.7: ref_mag=13.00 +/- 0.02 new_mean_mag=13.0165 delta=-0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:46:43.38 -02:12:58.0: ref_mag=12.13 +/- 0.01 new_mean_mag=12.0991 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:47:12.20 -03:24:39.7: ref_mag=12.98 +/- 0.02 new_mean_mag=12.9024 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:49:05.71 +03:09:11.6: ref_mag=13.35 +/- 0.03 new_mean_mag=13.5947 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:15:31.22 +01:55:46.3: 13.22 +/- 0.03 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 21:46:45.73 +00:44:29.4: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter REJECTED candidate at 21:46:45.73 +00:44:29.4: ref_mag=13.39 +/- 0.03 new_mean_mag=13.3930 delta=0.00 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:15:31.22 +01:55:46.3: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter REJECTED candidate at 22:15:31.22 +01:55:46.3: ref_mag=13.22 +/- 0.02 new_mean_mag=13.2662 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:30:23.15 -04:48:53.2: 13.27 +/- 0.05 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:41:37.42 +00:44:05.2: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:29:24.66 -03:13:58.4: 13.54 +/- 0.05 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:25:52.00 +02:28:27.9: 13.65 +/- 0.05 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:37:19.26 -00:08:50.4: 13.73 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:24:26.08 -06:00:56.2: 13.15 +/- 0.04 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:39:00.37 +01:00:49.5: 13.75 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:35:14.93 -02:15:52.9: 13.49 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-23-17_20.00sec_4.90C_LIGHT_1013.fits at 22:10:19.16 -02:17:28.0: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:37:19.26 -00:08:50.4: 13.74 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:39:00.37 +01:00:49.5: 13.59 +/- 0.05 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:24:26.08 -06:00:56.2: 13.18 +/- 0.04 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:35:14.93 -02:15:52.9: 13.62 +/- 0.06 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:29:24.66 -03:13:58.4: 13.53 +/- 0.05 detection
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:25:52.00 +02:28:27.9: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry reference-image weighted average: 13.66 +/- 0.04
Forced photometry filter REJECTED candidate at 22:37:19.26 -00:08:50.4: ref_mag=13.74 +/- 0.04 new_mean_mag=13.6969 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:30:23.15 -04:48:53.2: 13.28 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 22:39:00.37 +01:00:49.5: ref_mag=13.66 +/- 0.04 new_mean_mag=13.6377 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:24:26.08 -06:00:56.2: ref_mag=13.16 +/- 0.03 new_mean_mag=13.3947 delta=-0.23 (need > 0.90)
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Forced photometry filter REJECTED candidate at 22:29:24.66 -03:13:58.4: ref_mag=13.53 +/- 0.04 new_mean_mag=13.5023 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:25:52.00 +02:28:27.9: ref_mag=13.64 +/- 0.04 new_mean_mag=13.8041 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:35:14.93 -02:15:52.9: ref_mag=13.55 +/- 0.04 new_mean_mag=13.5624 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:41:37.42 +00:44:05.2: 15.66 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter REJECTED candidate at 22:30:23.15 -04:48:53.2: ref_mag=13.27 +/- 0.03 new_mean_mag=13.3768 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Aqr-02-Q1b1x1_2026-07-21_05-24-02_20.00sec_5.00C_LIGHT_1014.fits at 22:10:19.16 -02:17:28.0: 15.92 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out54847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54918.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 53973_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 53973_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 53974_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 53974_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 53979_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 53979_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 53980_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 53980_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54151_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54151_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
**** FOUND 22:43:10.28 -06:58:30.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54183_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54183_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
**** FOUND 22:33:54.54 -01:34:14.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54204_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54204_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54410_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54410_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54419_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54419_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54478_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54478_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54539_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54539_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
**** FOUND 22:23:38.00 -07:10:52.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54544_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54544_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54557_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54557_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54621_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54621_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54669_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54669_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54690_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54690_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54696_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54696_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54702_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54702_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54750_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54750_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks
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Considering the candidate 54756_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241
The candidate 54756_fd_Aqr-02-Q1b1x1_2026-09-01_01-13-18_20.00sec_0.00C_LIGHTs_0241 did not pass the final checks