This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR
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 09.4416 2461200.9416 12.05 21:31:30.49 -09:29:13.0
43.61566 -39.76288 galactic Cap Second-epoch detections are separated by 1.7" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.306 Unitas 0 -0 0 12.1 0 -0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:31:30.49 -09:29:13.0: 15.21 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:31:30.49 -09:29:13.0: 15.24 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 09.4416* 21 31 30.49 -09 29 13.0 12.1 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461200.9416,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260609.4416 12.05CV 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 09.4416 2461200.9416 11.91 21:04:42.37 -09:28:21.2
39.88869 -33.86398 galactic Aqr Second-epoch detections are separated by 1.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.287 Nephthys -0 1 1 12.1 -0 -0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:04:42.37 -09:28:21.2: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:04:42.37 -09:28:21.2: 15.03 +/- 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,2461200.9416,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260609.4416 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 09.4416 2461200.9416 12.62 21:46:44.81 -09:04:52.7
46.45496 -42.88662 galactic Cap Second-epoch detections are separated by 2.1" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.389 Industria 0 -0 0 12.8 0 0
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:46:44.81 -09:04:52.7: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:46:44.81 -09:04:52.7: 15.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 09.4416* 21 46 44.81 -09 04 52.7 12.6 U Cap 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461200.9416,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260609.4416 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
First image: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Last image: 2461200.94190522 09.06.2026 10:36:10.611 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.22
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 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): 6855
Objects passed selection criteria: 6839
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 5150.75
Average stars matched: 5066.25 (98.3595 %)
Memory usage VmPeak: 112744 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 9 07:53:31 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
First image: 2461177.87809874 17.05.2026 09:04:17.731 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Last image: 2461200.94190522 09.06.2026 10:36:10.611 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.00
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 20 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): 33998
Objects passed selection criteria: 33962
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 27333.8
Average stars matched: 26528.2 (97.0531 %)
Memory usage VmPeak: 137148 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 9 07:56:26 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.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: 2461200.94134703
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits exists and is non-empty
Saving wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits to local_wcs_cache/
'wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits'
wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits exists and is non-empty
Saving wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits to local_wcs_cache/
'wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits' -> 'local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits'
wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits exists and is non-empty
Saving wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits'
wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits exists and is non-empty
Saving wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits to local_wcs_cache/
'wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits' -> 'local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (1st reference image)
verification OK: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Image size: 941.9'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:33.187 -09:59:28.83 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
Image size: 940.8'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:55.877 -09:59:10.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:55.877 -09:59:10.33
Angular distance between the image centers 0.0932 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
Image size: 940.8'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:58.520 -09:58:39.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:58.520 -09:58:39.71
Angular distance between the image centers 0.1048 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:25:55.877 -09:59:10.33
Second-epoch second image center 21:25:58.520 -09:58:39.71
Angular distance between the image centers 0.01378 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits &> /tmp/tmp.alFOKCbatS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits &> /tmp/tmp.sQJjMiPCE0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits &> /tmp/tmp.NeLCwZywNL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits &> /tmp/tmp.Q6OMwNGYdV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
Found non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
The reference image (wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits) and catalog (wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat) found
'wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat' -> 'wcsmag.cat'
Read 7159 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 deg
Loaded 7438 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 5084 out of 5196 total matches.
Matched with Tycho-2 5196 out of 7159 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.642150
a=0.000000 b=1.000000 c=22.642150
From vast_summary.log: estimated ref. image limiting mag.: -8.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7159 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.0145 to 329.5552 deg, Dec -15.5597 to -4.2276 deg
Loaded 7438 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 5084 out of 5196 total matches.
Matched with Tycho-2 5196 out of 7159 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (aperture=7.4)
Read 7189 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0145 to 329.5561 deg, Dec -15.5598 to -4.2276 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.0145 to 329.5561 deg, Dec -15.5598 to -4.2276 deg
Loaded 7439 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 5086 out of 5190 total matches.
Matched with Tycho-2 5190 out of 7189 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits (aperture=7.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
3.3 pix Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.3 pix Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
3.6 pix fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
3.5 pix fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
3.3 pix wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.3 pix wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Limiting magnitude estimates:
14.4 mag. Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
14.4 mag. Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
13.7 mag. fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
12.6 mag. fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 10.4 (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.alFOKCbatS (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=329, passed=7159
Got 7159 stars (including 6821 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
util/solve_plate_with_UCAC5 got 7159 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits N_match=935 sigma_overall_arcsec=0.283 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.235 sigma_q4_arcsec=0.258 n_q1=280 n_q2=199 n_q3=264 n_q4=192 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -region wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.sQJjMiPCE0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=325, passed=7189
Got 7189 stars (including 6859 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat
util/solve_plate_with_UCAC5 got 7189 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 935 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits N_match=935 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.318 sigma_q3_arcsec=0.262 sigma_q4_arcsec=0.253 n_q1=283 n_q2=199 n_q3=260 n_q4=193 worst_quadrant_to_overall_ratio=1.112
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -region wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NeLCwZywNL (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_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.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_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=225, passed=4213
Got 4213 stars (including 3985 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat
util/solve_plate_with_UCAC5 got 4213 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 4110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 4110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 4110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits N_match=933 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.302 sigma_q4_arcsec=0.267 n_q1=256 n_q2=226 n_q3=252 n_q4=199 worst_quadrant_to_overall_ratio=1.218
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.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.Q6OMwNGYdV (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_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.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_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=102, passed=2156
Got 2156 stars (including 2053 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat
util/solve_plate_with_UCAC5 got 2156 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.5 to -4.4)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 2104 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.5 to -4.4)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 2102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 2102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 919 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits N_match=919 sigma_overall_arcsec=0.325 sigma_q1_arcsec=0.419 sigma_q2_arcsec=0.396 sigma_q3_arcsec=0.271 sigma_q4_arcsec=0.259 n_q1=219 n_q2=238 n_q3=237 n_q4=225 worst_quadrant_to_overall_ratio=1.288
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.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-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits sigma_overall=0.283 worst_q_ratio=1.198
ref2=Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits sigma_overall=0.286 worst_q_ratio=1.112
new1=fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits sigma_overall=0.350 worst_q_ratio=1.218
new2=fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits sigma_overall=0.325 worst_q_ratio=1.288
reference average sigma_overall=0.2845 worst_q_ratio=1.155
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428_astrometric_residuals.png (935 matched stars from wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429_astrometric_residuals.png (935 matched stars from wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350_astrometric_residuals.png (933 matched stars from wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351_astrometric_residuals.png (919 matched stars from wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits'
Saving fully-calibrated image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits'
Preparing the HTML report for the field Aqr-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aqr-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.cat to cache
SExtractor catalog cache: saved Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Creating symlink local_wcs_cache/wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
Creating symlink local_wcs_cache/wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits exists and is non-empty
wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits exists and is non-empty
wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits exists and is non-empty
wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (1st reference image)
verification OK: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Image size: 941.9'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:33.187 -09:59:28.83 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits (1st new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
Image size: 940.8'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:55.877 -09:59:10.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:55.877 -09:59:10.33
Angular distance between the image centers 0.0932 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits (2nd new image)
verification OK: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
Image size: 940.8'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 21:25:58.520 -09:58:39.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:25:33.187 -09:59:28.83
Second-epoch image center 21:25:58.520 -09:58:39.71
Angular distance between the image centers 0.1048 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 21:25:55.877 -09:59:10.33
Second-epoch second image center 21:25:58.520 -09:58:39.71
Angular distance between the image centers 0.01378 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits &> /tmp/tmp.YbDdGaQoYA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits &> /tmp/tmp.nFeugtSUtX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits &> /tmp/tmp.IlnsJw7COh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits &> /tmp/tmp.gyv2xfnyAu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
Calibrating the magnitude scale
Found non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.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-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
Found non-empty wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits and wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
The reference image (wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits) and catalog (wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat) found
'wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat' -> 'wcsmag.cat'
Read 36787 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 deg
Loaded 7455 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 5625 out of 6011 total matches.
Matched with Tycho-2 6011 out of 36787 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.521200
a=0.000000 b=1.000000 c=22.521200
From vast_summary.log: estimated ref. image limiting mag.: -8.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36787 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.0030 to 329.5641 deg, Dec -15.5697 to -4.2276 deg
Loaded 7455 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 5625 out of 6011 total matches.
Matched with Tycho-2 6011 out of 36787 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits (aperture=6.1)
Read 37049 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 313.0031 to 329.5643 deg, Dec -15.5699 to -4.2276 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 313.0031 to 329.5643 deg, Dec -15.5699 to -4.2276 deg
Loaded 7455 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 5641 out of 6012 total matches.
Matched with Tycho-2 6012 out of 37049 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits:
Forced-photometry filter: calibrated wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -> calib.txt_param_ref_wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
3.1 pix Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.1 pix Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
3.2 pix fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
3.1 pix fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
3.1 pix wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
3.1 pix wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Limiting magnitude estimates:
14.5 mag. Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
14.5 mag. Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
13.9 mag. fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
13.0 mag. fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.YbDdGaQoYA (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1449, passed=36780
Got 36780 stars (including 35283 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat
util/solve_plate_with_UCAC5 got 36780 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 35505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 35507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 35508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits N_match=936 sigma_overall_arcsec=0.300 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.353 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.318 n_q1=272 n_q2=191 n_q3=280 n_q4=193 worst_quadrant_to_overall_ratio=1.178
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits -region wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nFeugtSUtX (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits' -> 'wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS_IMAGE_NAME=wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS-calibrated image found: wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
Checking if the catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits alredy exist and is non-empty...
Catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits
WCS catalog name: wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1439, passed=37041
Got 37041 stars (including 35552 good ones) from the SExtractor catalog wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat
util/solve_plate_with_UCAC5 got 37041 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 35884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 35882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 35886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 940 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits N_match=940 sigma_overall_arcsec=0.290 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.314 sigma_q3_arcsec=0.276 sigma_q4_arcsec=0.252 n_q1=274 n_q2=196 n_q3=275 n_q4=195 worst_quadrant_to_overall_ratio=1.080
The image catalog is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits -region wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IlnsJw7COh (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_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.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_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=825, passed=23096
Got 23096 stars (including 22241 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat
util/solve_plate_with_UCAC5 got 23096 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 22577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 22580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 22580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits N_match=928 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.443 sigma_q2_arcsec=0.378 sigma_q3_arcsec=0.309 sigma_q4_arcsec=0.265 n_q1=240 n_q2=224 n_q3=259 n_q4=205 worst_quadrant_to_overall_ratio=1.271
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.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.gyv2xfnyAu (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_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.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_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
WCS_IMAGE_NAME=wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
WCS-calibrated image found: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
Checking if the catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits alredy exist and is non-empty...
Catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat corresponding to the image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
WCS catalog name: wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=348, passed=13289
Got 13289 stars (including 12930 good ones) from the SExtractor catalog wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat
util/solve_plate_with_UCAC5 got 13289 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 13024 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 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 13022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 13022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 921 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits N_match=921 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.411 sigma_q2_arcsec=0.386 sigma_q3_arcsec=0.293 sigma_q4_arcsec=0.270 n_q1=204 n_q2=231 n_q3=245 n_q4=241 worst_quadrant_to_overall_ratio=1.250
The image catalog is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits -region wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.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-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.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_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-35-22_20.00sec_-0.00C_LIGHTs_0350.fits
Saving fully-calibrated image wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.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_2026-06-09_CI_Aqr-03-Q1b1x1_074914_TTUQ1b1x1_3842386_tQQIXjlR/wcs_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351.fits
Preparing the HTML report for the field Aqr-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:31:30.49 -09:29:13.0: 15.21 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:32:40.52 -14:12:19.7: 11.80 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:38:57.31 -08:15:20.2: 12.65 +/- 0.04 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:20:14.53 -06:48:50.1: 11.83 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:46:44.81 -09:04:52.7: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:43:34.58 -10:00:05.9: 9.68 +/- 0.00 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:36:09.79 -06:01:23.5: 12.01 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-04-17_20.00sec_-0.00C_LIGHTs_0428.fits at 21:04:42.37 -09:28:21.2: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:31:30.49 -09:29:13.0: 15.24 +/- 99.00 upperlimit
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:20:14.53 -06:48:50.1: 11.79 +/- 0.02 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:32:40.52 -14:12:19.7: 11.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry filter REJECTED candidate at 21:20:14.53 -06:48:50.1: ref_mag=11.81 +/- 0.01 new_mean_mag=12.2889 delta=-0.48 (need > 0.90)
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Forced photometry filter REJECTED candidate at 21:32:40.52 -14:12:19.7: ref_mag=11.83 +/- 0.01 new_mean_mag=12.1124 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:38:57.31 -08:15:20.2: 12.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.03
Forced photometry filter REJECTED candidate at 21:38:57.31 -08:15:20.2: ref_mag=12.67 +/- 0.03 new_mean_mag=12.9781 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:43:34.58 -10:00:05.9: 9.67 +/- 0.00 detection
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:46:44.81 -09:04:52.7: 15.10 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 9.67 +/- 0.00
Forced photometry filter REJECTED candidate at 21:43:34.58 -10:00:05.9: ref_mag=9.67 +/- 0.00 new_mean_mag=9.7609 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:36:09.79 -06:01:23.5: 11.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter REJECTED candidate at 21:36:09.79 -06:01:23.5: ref_mag=12.00 +/- 0.01 new_mean_mag=12.6200 delta=-0.62 (need > 0.90)
Forced photometry on wcs_Aqr-03-Q1b1x1_2026-05-17_04-05-01_20.00sec_-0.00C_LIGHTs_0429.fits at 21:04:42.37 -09:28:21.2: 15.03 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out53022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53045.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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: 4s
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Considering the candidate 52978_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
The candidate 52978_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351 did not pass the final checks
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Considering the candidate 52983_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
The candidate 52983_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52984_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
The candidate 52984_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52988_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
The candidate 52988_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53022_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
Preparing report for the candidate 53022_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
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Considering the candidate 53027_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
Preparing report for the candidate 53027_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
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Considering the candidate 53045_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
Preparing report for the candidate 53045_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53056_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
The candidate 53056_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53061_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351
The candidate 53061_fd_Aqr-03-Q1b1x1_2026-06-09_05-36-10_20.00sec_0.00C_LIGHTs_0351 did not pass the final checks