This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 17.3838 2461208.8838 11.46 22:03:51.06 -08:39:37.2
49.90764 -46.34998 galactic Aqr Second-epoch detections are separated by 1.1" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.354 Eleonora -1 -0 1 11.5 -0 -0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:03:51.06 -08:39:37.2: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:03:51.06 -08:39:37.2: 15.04 +/- 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,2461208.8838,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260617.3838 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 17.3838 2461208.8838 12.18 22:23:11.25 -10:51:23.2
50.70433 -51.56958 galactic Aqr Second-epoch detections are separated by 0.6" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.100 Hekate 1 -0 1 12.4 0 0
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:23:11.25 -10:51:23.2: 15.17 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:23:11.25 -10:51:23.2: 15.17 +/- 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,2461208.8838,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260617.3838 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
First image: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Last image: 2461208.88412206 17.06.2026 09:12:58.146 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.05
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4636
Objects passed selection criteria: 4630
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 4230.75
Average stars matched: 3876.75 (91.6327 %)
Memory usage VmPeak: 110860 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jun 17 04:17:30 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
First image: 2461177.89902836 17.05.2026 09:34:26.050 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Last image: 2461208.88412206 17.06.2026 09:12:58.146 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 78
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.81
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: 23 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 28199
Objects passed selection criteria: 28151
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 26104.8
Average stars matched: 23731.5 (90.9087 %)
Memory usage VmPeak: 130932 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jun 17 04:20:18 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.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: 2461208.88356796
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits exists and is non-empty
Saving wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits'
wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
Saving wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits to local_wcs_cache/
'wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits'
wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits exists and is non-empty
Saving wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits to local_wcs_cache/
'wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits' -> 'local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Image size: 942.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:06.962 -09:59:19.64 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
Image size: 937.3'x624.2' 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: 22:17:08.551 -09:59:44.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:08.551 -09:59:44.07
Angular distance between the image centers 0.0094 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
Image size: 937.3'x624.2' 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: 22:17:11.454 -09:59:04.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:11.454 -09:59:04.26
Angular distance between the image centers 0.0189 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:17:08.551 -09:59:44.07
Second-epoch second image center 22:17:11.454 -09:59:04.26
Angular distance between the image centers 0.01625 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits &> /tmp/tmp.g15BRH1XDt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.TJq8FmG13x
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits &> /tmp/tmp.vphUQdePWj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits &> /tmp/tmp.kTaB6YsK7L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat' -> 'wcsmag.cat'
Read 4529 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 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 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 deg
Loaded 5486 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): 3405 out of 3455 total matches.
Matched with Tycho-2 3455 out of 4529 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.442200
a=0.000000 b=1.000000 c=22.442200
From vast_summary.log: estimated ref. image limiting mag.: -8.05
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.39
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 4529 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 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 325.9175 to 342.3809 deg, Dec -15.5885 to -4.2887 deg
Loaded 5486 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): 3405 out of 3455 total matches.
Matched with Tycho-2 3455 out of 4529 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (aperture=6.1)
Read 4507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.9176 to 342.3811 deg, Dec -15.5918 to -4.2887 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 325.9176 to 342.3811 deg, Dec -15.5918 to -4.2887 deg
Loaded 5486 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): 3392 out of 3444 total matches.
Matched with Tycho-2 3444 out of 4507 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
2.4 pix fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
2.3 pix fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
2.4 pix wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Limiting magnitude estimates:
14.4 mag. Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
14.4 mag. Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
14.6 mag. fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
14.7 mag. fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.g15BRH1XDt (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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=254, passed=4529
Got 4529 stars (including 4272 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
util/solve_plate_with_UCAC5 got 4529 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 4460 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 4459 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 883 matched stars entering correct_measured_positions(), 4459 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 883 stars left (next iteration limit 971)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits N_match=883 sigma_overall_arcsec=0.292 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.316 sigma_q3_arcsec=0.250 sigma_q4_arcsec=0.318 n_q1=255 n_q2=171 n_q3=261 n_q4=196 worst_quadrant_to_overall_ratio=1.090
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -region wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TJq8FmG13x (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-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=252, passed=4507
Got 4507 stars (including 4252 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 4507 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 4429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 4429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 4429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 881 stars left (next iteration limit 969)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits N_match=881 sigma_overall_arcsec=0.285 sigma_q1_arcsec=0.282 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.234 sigma_q4_arcsec=0.302 n_q1=256 n_q2=169 n_q3=258 n_q4=198 worst_quadrant_to_overall_ratio=1.217
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.vphUQdePWj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=358, passed=6127
Got 6127 stars (including 5763 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat
util/solve_plate_with_UCAC5 got 6127 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 893 matched stars entering correct_measured_positions(), 886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 893 matched stars entering correct_measured_positions(), 6051 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 893 matched stars entering correct_measured_positions(), 6052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 893 matched stars entering correct_measured_positions(), 6052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 893 stars left (next iteration limit 982)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits N_match=893 sigma_overall_arcsec=0.380 sigma_q1_arcsec=0.274 sigma_q2_arcsec=0.477 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.432 n_q1=241 n_q2=217 n_q3=228 n_q4=207 worst_quadrant_to_overall_ratio=1.255
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kTaB6YsK7L (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=366, passed=6068
Got 6068 stars (including 5697 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat
util/solve_plate_with_UCAC5 got 6068 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 6004 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 6001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 6001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 891 stars left (next iteration limit 980)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits N_match=891 sigma_overall_arcsec=0.396 sigma_q1_arcsec=0.298 sigma_q2_arcsec=0.472 sigma_q3_arcsec=0.382 sigma_q4_arcsec=0.492 n_q1=242 n_q2=214 n_q3=223 n_q4=212 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits sigma_overall=0.292 worst_q_ratio=1.090
ref2=Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits sigma_overall=0.285 worst_q_ratio=1.217
new1=fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits sigma_overall=0.380 worst_q_ratio=1.255
new2=fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits sigma_overall=0.396 worst_q_ratio=1.241
reference average sigma_overall=0.2885 worst_q_ratio=1.1535
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446_astrometric_residuals.png (883 matched stars from wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447_astrometric_residuals.png (881 matched stars from wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411_astrometric_residuals.png (893 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412_astrometric_residuals.png (891 matched stars from wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits'
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits'
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:03:51.06 -08:39:37.2: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:29:00.03 -09:56:39.7: 11.61 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:09:00.00 -09:37:19.5: 11.61 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:21:00.93 -14:05:01.4: 11.82 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:05:36.93 -09:52:54.6: 11.47 +/- 0.01 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:03:51.06 -08:39:37.2: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:09:00.00 -09:37:19.5: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Forced photometry filter REJECTED candidate at 22:09:00.00 -09:37:19.5: ref_mag=11.62 +/- 0.01 new_mean_mag=11.5844 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:21:00.93 -14:05:01.4: 11.82 +/- 0.02 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:05:36.93 -09:52:54.6: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Forced photometry filter REJECTED candidate at 22:21:00.93 -14:05:01.4: ref_mag=11.82 +/- 0.01 new_mean_mag=11.5286 delta=0.29 (need > 0.90)
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Forced photometry filter REJECTED candidate at 22:05:36.93 -09:52:54.6: ref_mag=11.46 +/- 0.01 new_mean_mag=11.4840 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:29:00.03 -09:56:39.7: 11.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Forced photometry filter REJECTED candidate at 22:29:00.03 -09:56:39.7: ref_mag=11.62 +/- 0.01 new_mean_mag=11.4596 delta=0.16 (need > 0.90)
Adding exclusion_list_local.txt__out20238.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20238_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
Preparing report for the candidate 20238_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20240_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 20240_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20242_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 20242_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20245_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 20245_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20248_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 20248_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:03:51.06 -08:39:37.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.cat to cache
SExtractor catalog cache: saved Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Creating symlink local_wcs_cache/wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits exists and is non-empty
wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits exists and is non-empty
wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (1st reference image)
verification OK: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Image size: 942.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:06.962 -09:59:19.64 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits (1st new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
Image size: 937.3'x624.2' 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: 22:17:08.551 -09:59:44.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:08.551 -09:59:44.07
Angular distance between the image centers 0.0094 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits (2nd new image)
verification OK: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
Image size: 937.3'x624.2' 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: 22:17:11.454 -09:59:04.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:06.962 -09:59:19.64
Second-epoch image center 22:17:11.454 -09:59:04.26
Angular distance between the image centers 0.0189 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:17:08.551 -09:59:44.07
Second-epoch second image center 22:17:11.454 -09:59:04.26
Angular distance between the image centers 0.01625 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits &> /tmp/tmp.leku5QkGsw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.cbv2Mkx2RE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits &> /tmp/tmp.MDc6av9dfo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits &> /tmp/tmp.RqX7hr5SOn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
Found non-empty wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits and wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
The reference image (wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits) and catalog (wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat) found
'wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat' -> 'wcsmag.cat'
Read 27177 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 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 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 deg
Loaded 5550 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): 4272 out of 4485 total matches.
Matched with Tycho-2 4485 out of 27177 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.308200
a=0.000000 b=1.000000 c=22.308200
From vast_summary.log: estimated ref. image limiting mag.: -7.81
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27177 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 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 325.8701 to 342.4551 deg, Dec -15.5885 to -4.2463 deg
Loaded 5550 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): 4272 out of 4485 total matches.
Matched with Tycho-2 4485 out of 27177 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits (aperture=5.0)
Read 27357 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.8701 to 342.4399 deg, Dec -15.6108 to -4.2411 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 325.8701 to 342.4399 deg, Dec -15.6108 to -4.2411 deg
Loaded 5555 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): 4272 out of 4487 total matches.
Matched with Tycho-2 4487 out of 27357 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits:
Forced-photometry filter: calibrated wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -> calib.txt_param_ref_wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 32 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
2.3 pix fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
2.2 pix fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
2.4 pix wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
2.4 pix wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Limiting magnitude estimates:
14.5 mag. Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
14.5 mag. Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
14.9 mag. fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
14.9 mag. fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 13.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.leku5QkGsw (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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.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-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=866, passed=27173
Got 27173 stars (including 26256 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat
util/solve_plate_with_UCAC5 got 27173 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 26753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 26754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 882 matched stars entering correct_measured_positions(), 26754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 882 stars left (next iteration limit 970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits N_match=882 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.285 sigma_q2_arcsec=0.326 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.338 n_q1=253 n_q2=169 n_q3=270 n_q4=190 worst_quadrant_to_overall_ratio=1.150
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits -region wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cbv2Mkx2RE (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-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.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-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=827, passed=27350
Got 27350 stars (including 26485 good ones) from the SExtractor catalog wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 27350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010474 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 26942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 26945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 881 matched stars entering correct_measured_positions(), 26945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 881 stars left (next iteration limit 969)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits N_match=881 sigma_overall_arcsec=0.289 sigma_q1_arcsec=0.264 sigma_q2_arcsec=0.390 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.304 n_q1=253 n_q2=170 n_q3=266 n_q4=192 worst_quadrant_to_overall_ratio=1.351
The image catalog is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MDc6av9dfo (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1441, passed=34322
Got 34322 stars (including 32845 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat
util/solve_plate_with_UCAC5 got 34322 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 885 matched stars entering correct_measured_positions(), 878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 885 matched stars entering correct_measured_positions(), 33884 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
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 885 matched stars entering correct_measured_positions(), 33884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 885 matched stars entering correct_measured_positions(), 33884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 885 stars left (next iteration limit 973)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits N_match=885 sigma_overall_arcsec=0.415 sigma_q1_arcsec=0.329 sigma_q2_arcsec=0.513 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.475 n_q1=248 n_q2=205 n_q3=222 n_q4=210 worst_quadrant_to_overall_ratio=1.235
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.RqX7hr5SOn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
WCS-calibrated image found: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
Checking if the catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat corresponding to the image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
WCS catalog name: wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1466, passed=34598
Got 34598 stars (including 33095 good ones) from the SExtractor catalog wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat
util/solve_plate_with_UCAC5 got 34598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 34179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 34178 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 34178 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 880 stars left (next iteration limit 968)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits N_match=880 sigma_overall_arcsec=0.406 sigma_q1_arcsec=0.296 sigma_q2_arcsec=0.502 sigma_q3_arcsec=0.367 sigma_q4_arcsec=0.509 n_q1=244 n_q2=200 n_q3=221 n_q4=215 worst_quadrant_to_overall_ratio=1.254
The image catalog is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits -region wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-10_20.00sec_4.90C_LIGHT_0411.fits
Saving fully-calibrated image wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Aqr-04-Q2b1x1_041510_TTUQ2b1x1_1489151_qf4PUTP1/wcs_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412.fits
Preparing the HTML report for the field Aqr-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:56:23.34 -11:50:36.1: 12.22 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:27:18.65 -09:24:59.9: 13.39 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:06:15.26 -08:17:10.5: 14.00 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:10:49.64 -07:56:35.4: 13.57 +/- 0.09 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:53:44.83 -12:38:06.3: 13.52 +/- 0.10 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:55:05.73 -13:32:22.4: 14.32 +/- 0.21 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:52:13.30 -13:32:07.5: 14.03 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:16:01.35 -06:53:46.6: 13.51 +/- 0.08 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:50:44.71 -12:34:11.2: 13.11 +/- 0.07 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:12:19.40 -10:03:21.3: 12.47 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:23.34 -11:50:36.1: 12.24 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:50:44.71 -12:34:11.2: 13.35 +/- 0.09 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:10:49.64 -07:56:35.4: 13.55 +/- 0.08 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:27:18.65 -09:24:59.9: 13.37 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 21:56:23.34 -11:50:36.1: ref_mag=12.23 +/- 0.02 new_mean_mag=12.4816 delta=-0.25 (need > 0.90)
Forced photometry reference-image weighted average: 13.20 +/- 0.06
Forced photometry filter REJECTED candidate at 21:50:44.71 -12:34:11.2: ref_mag=13.20 +/- 0.06 new_mean_mag=13.4647 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:06:15.26 -08:17:10.5: 14.05 +/- 0.13 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:12:19.40 -10:03:21.3: 12.43 +/- 0.03 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:52:13.30 -13:32:07.5: 14.41 +/- 0.24 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.06
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:16:01.35 -06:53:46.6: 13.64 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
Forced photometry filter REJECTED candidate at 22:10:49.64 -07:56:35.4: ref_mag=13.56 +/- 0.06 new_mean_mag=13.7867 delta=-0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:27:18.65 -09:24:59.9: ref_mag=13.38 +/- 0.05 new_mean_mag=13.6968 delta=-0.31 (need > 0.90)
Forced photometry reference-image weighted average: 14.02 +/- 0.09
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Forced photometry reference-image weighted average: 14.16 +/- 0.14
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:55:05.73 -13:32:22.4: 14.12 +/- 0.17 detection
Forced photometry filter REJECTED candidate at 22:06:15.26 -08:17:10.5: ref_mag=14.02 +/- 0.09 new_mean_mag=14.0619 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:12:19.40 -10:03:21.3: ref_mag=12.45 +/- 0.02 new_mean_mag=12.8301 delta=-0.38 (need > 0.90)
Forced photometry reference-image weighted average: 13.57 +/- 0.06
Forced photometry filter REJECTED candidate at 21:52:13.30 -13:32:07.5: ref_mag=14.16 +/- 0.14 new_mean_mag=14.0982 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:16:01.35 -06:53:46.6: ref_mag=13.57 +/- 0.06 new_mean_mag=13.8798 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:44.83 -12:38:06.3: 13.55 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.13
Forced photometry filter REJECTED candidate at 21:55:05.73 -13:32:22.4: ref_mag=14.20 +/- 0.13 new_mean_mag=14.0073 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.53 +/- 0.07
Forced photometry filter REJECTED candidate at 21:53:44.83 -12:38:06.3: ref_mag=13.53 +/- 0.07 new_mean_mag=13.6646 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:30:59.79 -14:00:10.8: 13.61 +/- 0.10 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:23:11.25 -10:51:23.2: 15.17 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:52:31.32 -13:22:07.5: 12.82 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:57:58.35 -14:05:44.4: 13.68 +/- 0.12 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:31:37.44 -13:34:17.1: 13.98 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:52:57.79 -13:32:07.1: 14.01 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:56:46.20 -13:00:43.1: 13.87 +/- 0.13 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 22:03:55.19 -14:03:58.7: 14.06 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:57:02.12 -12:20:47.1: 14.47 +/- 0.22 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:56:45.52 -14:10:46.6: 14.06 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:23:11.25 -10:51:23.2: 15.17 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:30:59.79 -14:00:10.8: 14.00 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.08
Forced photometry filter REJECTED candidate at 22:30:59.79 -14:00:10.8: ref_mag=13.74 +/- 0.08 new_mean_mag=13.9920 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:52:31.32 -13:22:07.5: 12.93 +/- 0.06 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:31:37.44 -13:34:17.1: 13.85 +/- 0.13 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:46.20 -13:00:43.1: 14.13 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 22:03:55.19 -14:03:58.7: 13.89 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:57:58.35 -14:05:44.4: 13.88 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:57:02.12 -12:20:47.1: 13.94 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:52:57.79 -13:32:07.1: 14.20 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.10
Forced photometry reference-image weighted average: 12.87 +/- 0.04
Forced photometry reference-image weighted average: 13.91 +/- 0.10
Forced photometry reference-image weighted average: 13.77 +/- 0.09
Forced photometry reference-image weighted average: 14.08 +/- 0.12
Forced photometry reference-image weighted average: 13.96 +/- 0.10
Forced photometry filter REJECTED candidate at 21:56:46.20 -13:00:43.1: ref_mag=13.97 +/- 0.10 new_mean_mag=13.9854 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:52:31.32 -13:22:07.5: ref_mag=12.87 +/- 0.04 new_mean_mag=12.9401 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:31:37.44 -13:34:17.1: ref_mag=13.91 +/- 0.10 new_mean_mag=13.9608 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:57:02.12 -12:20:47.1: ref_mag=14.08 +/- 0.12 new_mean_mag=14.0148 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:57:58.35 -14:05:44.4: ref_mag=13.77 +/- 0.09 new_mean_mag=13.8521 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:03:55.19 -14:03:58.7: ref_mag=13.96 +/- 0.10 new_mean_mag=13.9909 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.09 +/- 0.13
Forced photometry filter REJECTED candidate at 21:52:57.79 -13:32:07.1: ref_mag=14.09 +/- 0.13 new_mean_mag=13.8648 delta=0.22 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:56:45.52 -14:10:46.6: 14.09 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.12
Forced photometry filter REJECTED candidate at 21:56:45.52 -14:10:46.6: ref_mag=14.07 +/- 0.12 new_mean_mag=14.0166 delta=0.06 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:50:49.34 -13:46:02.4: 13.94 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:53:37.87 -12:47:00.5: 14.27 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:54:14.46 -11:51:54.0: 14.00 +/- 0.16 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:49:42.87 -12:29:01.3: 14.39 +/- 0.24 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:53:18.55 -05:45:50.7: 13.92 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:49:19.20 -11:24:09.9: 13.89 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:50:55.02 -14:11:32.2: 14.27 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:51:07.44 -14:09:32.6: 14.08 +/- 0.19 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:51:04.83 -08:30:32.1: 13.98 +/- 0.14 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:50:49.34 -13:46:02.4: 14.43 +/- 0.25 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:37.87 -12:47:00.5: 14.27 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.14
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:54:14.46 -11:51:54.0: 14.12 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 21:50:49.34 -13:46:02.4: ref_mag=14.09 +/- 0.14 new_mean_mag=13.9764 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:53:18.55 -05:45:50.7: 14.03 +/- 0.15 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:19.20 -11:24:09.9: 14.05 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.14
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:50:55.02 -14:11:32.2: 14.14 +/- 0.20 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:42.87 -12:29:01.3: 14.12 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 21:53:37.87 -12:47:00.5: ref_mag=14.27 +/- 0.14 new_mean_mag=14.0549 delta=0.21 (need > 0.90)
Forced photometry reference-image weighted average: 14.05 +/- 0.12
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:51:07.44 -14:09:32.6: 13.92 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 21:54:14.46 -11:51:54.0: ref_mag=14.05 +/- 0.12 new_mean_mag=14.0372 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.97 +/- 0.10
Forced photometry reference-image weighted average: 14.20 +/- 0.15
Forced photometry reference-image weighted average: 13.96 +/- 0.11
Forced photometry filter REJECTED candidate at 21:53:18.55 -05:45:50.7: ref_mag=13.97 +/- 0.10 new_mean_mag=13.8672 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:49:19.20 -11:24:09.9: ref_mag=13.96 +/- 0.11 new_mean_mag=13.9876 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:50:55.02 -14:11:32.2: ref_mag=14.20 +/- 0.15 new_mean_mag=14.0117 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 14.22 +/- 0.15
Forced photometry reference-image weighted average: 13.98 +/- 0.12
Forced photometry filter REJECTED candidate at 21:49:42.87 -12:29:01.3: ref_mag=14.22 +/- 0.15 new_mean_mag=13.8998 delta=0.33 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:51:07.44 -14:09:32.6: ref_mag=13.98 +/- 0.12 new_mean_mag=13.9829 delta=0.00 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:51:04.83 -08:30:32.1: 13.85 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.09
Forced photometry filter REJECTED candidate at 21:51:04.83 -08:30:32.1: ref_mag=13.90 +/- 0.09 new_mean_mag=13.9280 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:58:10.28 -07:20:47.8: 14.56 +/- 0.24 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-34-26_20.00sec_0.00C_LIGHTs_0446.fits at 21:49:54.58 -07:44:51.9: 14.48 +/- 0.23 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:58:10.28 -07:20:47.8: 14.17 +/- 0.17 detection
Forced photometry on wcs_Aqr-04-Q2b1x1_2026-05-17_04-35-12_20.00sec_-0.00C_LIGHTs_0447.fits at 21:49:54.58 -07:44:51.9: 14.59 +/- 0.26 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.14
Forced photometry filter REJECTED candidate at 21:58:10.28 -07:20:47.8: ref_mag=14.30 +/- 0.14 new_mean_mag=14.0778 delta=0.22 (need > 0.90)
Forced photometry reference-image weighted average: 14.53 +/- 0.17
Forced photometry filter REJECTED candidate at 21:49:54.58 -07:44:51.9: ref_mag=14.53 +/- 0.17 new_mean_mag=14.0301 delta=0.50 (need > 0.90)
Adding exclusion_list_local.txt__out32074.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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
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Considering the candidate 31938_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 31938_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 31939_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 31939_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 31940_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 31940_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 31944_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 31944_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 31946_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 31946_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 31947_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 31947_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 31948_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 31948_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 31949_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 31949_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 31952_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 31952_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 31955_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 31955_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32030_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32030_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
**** FOUND 22:03:51.07 -08:39:37.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 32074_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
Preparing report for the candidate 32074_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
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Considering the candidate 32235_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32235_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32366_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32366_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32380_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32380_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32427_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32427_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32445_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32445_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32489_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32489_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32522_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32522_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32528_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32528_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32541_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32541_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32559_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32559_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32560_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32560_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32572_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32572_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32577_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32577_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32601_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32601_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32643_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32643_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32647_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32647_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32677_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32677_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32759_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32759_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32781_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32781_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks
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Considering the candidate 32947_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412
The candidate 32947_fd_Aqr-04-Q2b1x1_2026-06-17_04-12-58_20.00sec_5.00C_LIGHT_0412 did not pass the final checks