This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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,2461290.7134,11.16,0.05,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 20260907.2134 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2134 2461290.7134 10.21 22:23:47.63 -34:53:07.4
9.85050 -57.62092 galactic PsA Second-epoch detections are separated by 0.6" and 5.4 pix
The object was found in VSX 5" NSV 25888
Type:
# Max. Min./Amp. JD0 Period
4.110 J 4.340 J M8
The object was not found in astcheck.
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:23:47.63 -34:53:07.4: 11.21 +/- 0.04 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:23:47.63 -34:53:07.4: 11.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.02
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 Lite
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
NSV 25888,2461290.7134,10.21,0.05,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
NSV 25888 20260907.2134 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.2134 2461290.7134 11.47 22:23:08.87 -34:17:56.4
10.95550 -57.51900 galactic PsA Second-epoch detections are separated by 0.5" and 5.4 pix
The object was found in VSX 1" ASAS J222309-3417.9
Type: MISC
# Max. Min./Amp. JD0 Period
12.140 V Y 0.600 V 2452005.50000 84.573486000000
The object was not found in astcheck.
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:23:08.87 -34:17:56.4: 12.37 +/- 0.12 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:23:08.87 -34:17:56.4: 12.48 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.08
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 Lite
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
ASAS J222309-3417.9,2461290.7134,11.47,0.05,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
ASAS J222309-3417.9 20260907.2134 11.47CV 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: 2461230.90518097 09.07.2026 09:43:17.636 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
First image: 2461230.90518097 09.07.2026 09:43:17.636 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Last image: 2461290.71372009 07.09.2026 05:07:35.416 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.85
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 1349
Objects passed selection criteria: 1348
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 1137
Average stars matched: 1034 (90.9411 %)
Memory usage VmPeak: 228420 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 00:09:37 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: 2461230.90518097 09.07.2026 09:43:17.636 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
First image: 2461230.90518097 09.07.2026 09:43:17.636 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Last image: 2461290.71372009 07.09.2026 05:07:35.416 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 24
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.50
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: 6 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 9214
Objects passed selection criteria: 9199
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 7854.25
Average stars matched: 7186.25 (91.4951 %)
Memory usage VmPeak: 235412 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 00:10:36 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
SExtractor catalog cache: saved PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.cat to cache
SExtractor catalog cache: saved PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.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/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.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: 2461290.71312757
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits exists and is non-empty
wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits exists and is non-empty
wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits exists and is non-empty
wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits (1st reference image)
verification OK: wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Image size: 937.5'x625.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 22:57:25.622 -34:00:40.75 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits (1st new image)
verification OK: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
Image size: 941.2'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:57:46.192 -34:01:01.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:57:25.622 -34:00:40.75
Second-epoch image center 22:57:46.192 -34:01:01.98
Angular distance between the image centers 0.0713 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits (2nd new image)
verification OK: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Image size: 941.2'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:57:43.595 -34:00:55.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:57:25.622 -34:00:40.75
Second-epoch image center 22:57:43.595 -34:00:55.56
Angular distance between the image centers 0.0622 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:57:46.192 -34:01:01.98
Second-epoch second image center 22:57:43.595 -34:00:55.56
Angular distance between the image centers 0.00915 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits &> /tmp/tmp.fwH2ZiPLXA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits &> /tmp/tmp.eMtUVUcIwj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits &> /tmp/tmp.h9Ds0BNQp3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits &> /tmp/tmp.op4I4iClow
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Calibrating the magnitude scale
Found non-empty wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.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_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits and wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.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_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits and wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat
Found non-empty wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits and wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat
The reference image (wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits) and catalog (wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat) found
'wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat' -> 'wcsmag.cat'
Read 1183 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 334.4424 to 353.9626 deg, Dec -39.1780 to -28.5199 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 334.4424 to 353.9626 deg, Dec -39.1780 to -28.5199 deg
Loaded 5070 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): 876 out of 882 total matches.
Matched with Tycho-2 882 out of 1183 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.897400
a=0.000000 b=1.000000 c=21.897400
From vast_summary.log: estimated ref. image limiting mag.: -8.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.05
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.05
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 1183 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 334.4424 to 353.9626 deg, Dec -39.1780 to -28.5199 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 334.4424 to 353.9626 deg, Dec -39.1780 to -28.5199 deg
Loaded 5070 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): 876 out of 882 total matches.
Matched with Tycho-2 882 out of 1183 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Forced-photometry filter: calibrated wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits -> calib.txt_param_ref_wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits (aperture=6.4)
Read 1486 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 334.4427 to 353.9628 deg, Dec -39.2404 to -28.5200 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 334.4427 to 353.9628 deg, Dec -39.2404 to -28.5200 deg
Loaded 5104 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): 1168 out of 1175 total matches.
Matched with Tycho-2 1175 out of 1486 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
Forced-photometry filter: calibrated wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits -> calib.txt_param_ref_wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
2.2 pix PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
3.7 pix fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
3.6 pix fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Limiting magnitude estimates:
13.0 mag. PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
13.3 mag. PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
12.5 mag. fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
12.5 mag. fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
All-image limiting magnitude estimate: 12.5 (SNR ) 10.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.fwH2ZiPLXA (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits' -> 'wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
WCS-calibrated image found: wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Checking if the catalog wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat corresponding to the image wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat corresponding to the image wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
WCS catalog name: wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=120, bad_region=0, passed=1183
Got 1183 stars (including 1063 good ones) from the SExtractor catalog wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat
util/solve_plate_with_UCAC5 got 1183 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 254 to 309 (Dec -39.2 to -28.5)
Done reading UCAC5 zone files...
Matched 1021 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1021 matched stars entering correct_measured_positions(), 1019 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1021 matched stars entering correct_measured_positions(), 1179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 254 to 309 (Dec -39.2 to -28.5)
Done reading UCAC5 zone files...
Matched 1021 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1021 matched stars entering correct_measured_positions(), 1177 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 1021 matched stars entering correct_measured_positions(), 1177 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 1021 stars left (next iteration limit 1123)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits N_match=1021 sigma_overall_arcsec=0.458 sigma_q1_arcsec=0.384 sigma_q2_arcsec=0.523 sigma_q3_arcsec=0.494 sigma_q4_arcsec=0.434 n_q1=269 n_q2=218 n_q3=285 n_q4=249 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits -region wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.eMtUVUcIwj (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits' -> 'wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
WCS_IMAGE_NAME=wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
WCS-calibrated image found: wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
Checking if the catalog wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat corresponding to the image wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits alredy exist and is non-empty...
Catalog wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat corresponding to the image wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
WCS catalog name: wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=145, bad_region=0, passed=1486
Got 1486 stars (including 1338 good ones) from the SExtractor catalog wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat
util/solve_plate_with_UCAC5 got 1486 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.2 to -28.5)
Done reading UCAC5 zone files...
Matched 1291 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1291 matched stars entering correct_measured_positions(), 1290 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1291 matched stars entering correct_measured_positions(), 1484 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.2 to -28.5)
Done reading UCAC5 zone files...
Matched 1291 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1291 matched stars entering correct_measured_positions(), 1484 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 1291 matched stars entering correct_measured_positions(), 1484 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 1291 stars left (next iteration limit 1420)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits N_match=1291 sigma_overall_arcsec=0.468 sigma_q1_arcsec=0.460 sigma_q2_arcsec=0.616 sigma_q3_arcsec=0.403 sigma_q4_arcsec=0.459 n_q1=351 n_q2=287 n_q3=344 n_q4=309 worst_quadrant_to_overall_ratio=1.316
The image catalog is written to wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits -region wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.h9Ds0BNQp3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
Checking if the catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
WCS catalog name: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=48, bad_region=0, passed=967
Got 967 stars (including 919 good ones) from the SExtractor catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 967 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.2)
Done reading UCAC5 zone files...
Matched 880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.2)
Done reading UCAC5 zone files...
Matched 881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 880 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 880 stars left (next iteration limit 966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=880 robust_rms=7.102 arcsec worst_quadrant_rms=15.654 arcsec
SIP_REFIT: SIP order 3 trial: matched=880 robust_rms=0.495 arcsec worst_quadrant_rms=0.554 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=880 robust_rms_before=1.005 arcsec robust_rms_before_corrected=0.428 arcsec robust_rms_after=0.495 arcsec worst_quadrant_rms_before=0.487 worst_quadrant_rms_after=0.554
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.487 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits N_match=880 sigma_overall_arcsec=0.437 sigma_q1_arcsec=0.446 sigma_q2_arcsec=0.534 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.354 n_q1=335 n_q2=191 n_q3=200 n_q4=154 worst_quadrant_to_overall_ratio=1.222
The image catalog is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits -region wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.op4I4iClow (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
WCS_IMAGE_NAME=wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
WCS-calibrated image found: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Checking if the catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat corresponding to the image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits alredy exist and is non-empty...
Catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat corresponding to the image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
WCS catalog name: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=54, bad_region=0, passed=939
Got 939 stars (including 884 good ones) from the SExtractor catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 939 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 850 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 850 matched stars entering correct_measured_positions(), 825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 850 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 848 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 848 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 848 stars left (next iteration limit 935)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=848 robust_rms=6.730 arcsec worst_quadrant_rms=21.823 arcsec
SIP_REFIT: SIP order 3 trial: matched=848 robust_rms=0.527 arcsec worst_quadrant_rms=0.626 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=848 robust_rms_before=0.930 arcsec robust_rms_before_corrected=0.446 arcsec robust_rms_after=0.527 arcsec worst_quadrant_rms_before=0.561 worst_quadrant_rms_after=0.626
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.561 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits N_match=848 sigma_overall_arcsec=0.449 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.603 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.386 n_q1=344 n_q2=189 n_q3=189 n_q4=126 worst_quadrant_to_overall_ratio=1.344
The image catalog is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits -region wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits to local_wcs_cache/
'wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits' -> 'local_wcs_cache/wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits'
Saving the final (post-refit) wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits to local_wcs_cache/
'wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits' -> 'local_wcs_cache/wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits'
Saving the final (post-refit) wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits to local_wcs_cache/
'wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits' -> 'local_wcs_cache/wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits'
Saving the final (post-refit) wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits to local_wcs_cache/
'wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits' -> 'local_wcs_cache/wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits sigma_overall=0.458 worst_q_ratio=1.142
ref2=PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits sigma_overall=0.468 worst_q_ratio=1.316
new1=fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits sigma_overall=0.437 worst_q_ratio=1.222
new2=fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits sigma_overall=0.449 worst_q_ratio=1.344
reference average sigma_overall=0.463 worst_q_ratio=1.229
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207_astrometric_residuals.png (1021 matched stars from wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403_astrometric_residuals.png (1291 matched stars from wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138_astrometric_residuals.png (880 matched stars from wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139_astrometric_residuals.png (848 matched stars from wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits'
Saving fully-calibrated image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits'
Preparing the HTML report for the field PsA-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:25:05.53 -34:12:33.3: 10.67 +/- 0.03 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:20:00.93 -34:39:06.5: 10.77 +/- 0.03 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:37:21.84 -37:43:27.2: 10.67 +/- 0.03 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:23:47.60 -34:53:07.1: 11.06 +/- 0.04 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:37:21.84 -37:43:27.2: 10.74 +/- 0.02 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:25:05.53 -34:12:33.3: 10.69 +/- 0.02 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:23:47.60 -34:53:07.1: 11.03 +/- 0.03 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:20:00.93 -34:39:06.5: 10.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.71 +/- 0.02
Forced photometry reference-image weighted average: 11.04 +/- 0.02
Forced photometry reference-image weighted average: 10.68 +/- 0.02
Forced photometry reference-image weighted average: 10.70 +/- 0.02
Forced photometry filter REJECTED candidate at 22:37:21.84 -37:43:27.2: ref_mag=10.71 +/- 0.02 new_mean_mag=10.2501 delta=0.46 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:47.60 -34:53:07.1: ref_mag=11.04 +/- 0.02 new_mean_mag=10.1451 delta=0.89 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:25:05.53 -34:12:33.3: ref_mag=10.68 +/- 0.02 new_mean_mag=10.2595 delta=0.42 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:20:00.93 -34:39:06.5: ref_mag=10.70 +/- 0.02 new_mean_mag=10.2393 delta=0.46 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20337_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 20337_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20339_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 20339_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
**** FOUND 22:54:18.68 -34:23:26.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20341_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 20341_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20342_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 20342_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20343_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 20343_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20155_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 20155_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
**** FOUND 22:47:50.11 -36:42:08.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field PsA-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
SExtractor catalog cache: saved PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.cat to cache
SExtractor catalog cache: saved PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Creating symlink local_wcs_cache/wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
Creating symlink local_wcs_cache/wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
Creating symlink local_wcs_cache/wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits exists and is non-empty
wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits exists and is non-empty
wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits exists and is non-empty
wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits (1st reference image)
verification OK: wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Image size: 937.5'x625.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 22:57:25.622 -34:00:40.75 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits (1st new image)
verification OK: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
Image size: 941.2'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:57:46.192 -34:01:01.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:57:25.622 -34:00:40.75
Second-epoch image center 22:57:46.192 -34:01:01.98
Angular distance between the image centers 0.0713 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits (2nd new image)
verification OK: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Image size: 941.2'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:57:43.595 -34:00:55.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:57:25.622 -34:00:40.75
Second-epoch image center 22:57:43.595 -34:00:55.56
Angular distance between the image centers 0.0622 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:57:46.192 -34:01:01.98
Second-epoch second image center 22:57:43.595 -34:00:55.56
Angular distance between the image centers 0.00915 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits &> /tmp/tmp.4I99yCc0Gf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits &> /tmp/tmp.B2dMRypyCj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits &> /tmp/tmp.yI7WfBlLvK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits &> /tmp/tmp.nazXp8bpSd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Calibrating the magnitude scale
Found non-empty wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.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_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits and wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.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_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits and wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat
Found non-empty wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits and wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat
The reference image (wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits) and catalog (wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat) found
'wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat' -> 'wcsmag.cat'
Read 9043 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 334.4155 to 354.1392 deg, Dec -39.2769 to -28.4989 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 334.4155 to 354.1392 deg, Dec -39.2769 to -28.4989 deg
Loaded 5175 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): 4151 out of 4206 total matches.
Matched with Tycho-2 4206 out of 9043 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.687300
a=0.000000 b=1.000000 c=21.687300
From vast_summary.log: estimated ref. image limiting mag.: -8.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.19
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9043 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 334.4155 to 354.1392 deg, Dec -39.2769 to -28.4989 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 334.4155 to 354.1392 deg, Dec -39.2769 to -28.4989 deg
Loaded 5175 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): 4151 out of 4206 total matches.
Matched with Tycho-2 4206 out of 9043 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Forced-photometry filter: calibrated wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits -> calib.txt_param_ref_wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits (aperture=4.7)
Read 10991 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 334.4156 to 354.1393 deg, Dec -39.2569 to -28.4575 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 334.4156 to 354.1393 deg, Dec -39.2569 to -28.4575 deg
Loaded 5179 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): 4121 out of 4191 total matches.
Matched with Tycho-2 4191 out of 10991 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
Forced-photometry filter: calibrated wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits -> calib.txt_param_ref_wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
2.1 pix PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
3.3 pix fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
3.3 pix fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Limiting magnitude estimates:
13.2 mag. PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
13.5 mag. PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
12.8 mag. fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
12.8 mag. fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.4I99yCc0Gf (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits' -> 'wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
WCS-calibrated image found: wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
Checking if the catalog wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat corresponding to the image wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat corresponding to the image wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits
WCS catalog name: wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=213, bad_region=0, passed=9042
Got 9042 stars (including 8816 good ones) from the SExtractor catalog wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat
util/solve_plate_with_UCAC5 got 9042 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4853 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 9042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4852 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 9042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 9042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4849 stars left (next iteration limit 5335)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits N_match=4849 sigma_overall_arcsec=0.589 sigma_q1_arcsec=0.567 sigma_q2_arcsec=0.607 sigma_q3_arcsec=0.662 sigma_q4_arcsec=0.518 n_q1=1367 n_q2=1073 n_q3=1245 n_q4=1164 worst_quadrant_to_overall_ratio=1.124
The image catalog is written to wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits -region wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.B2dMRypyCj (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits' -> 'wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
WCS_IMAGE_NAME=wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
WCS-calibrated image found: wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
Checking if the catalog wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat corresponding to the image wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits alredy exist and is non-empty...
Catalog wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat corresponding to the image wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits
WCS catalog name: wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=284, bad_region=0, passed=10990
Got 10990 stars (including 10688 good ones) from the SExtractor catalog wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat
util/solve_plate_with_UCAC5 got 10990 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4858 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 4855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 10990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4858 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 10990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 10990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4854 stars left (next iteration limit 5340)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits N_match=4854 sigma_overall_arcsec=0.536 sigma_q1_arcsec=0.515 sigma_q2_arcsec=0.667 sigma_q3_arcsec=0.507 sigma_q4_arcsec=0.505 n_q1=1375 n_q2=982 n_q3=1347 n_q4=1150 worst_quadrant_to_overall_ratio=1.246
The image catalog is written to wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits -region wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.yI7WfBlLvK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
Checking if the catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
WCS catalog name: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=138, bad_region=0, passed=5920
Got 5920 stars (including 5775 good ones) from the SExtractor catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 5920 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 4831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 5915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 5915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 5915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Excluding outliers - 4836 stars left (next iteration limit 5319)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4836 robust_rms=6.550 arcsec worst_quadrant_rms=20.250 arcsec
SIP_REFIT: SIP order 3 trial: matched=4836 robust_rms=1.064 arcsec worst_quadrant_rms=1.263 arcsec
SIP_REFIT: SIP order 5 trial: matched=4836 robust_rms=0.978 arcsec worst_quadrant_rms=1.106 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4836 robust_rms_before=1.383 arcsec robust_rms_before_corrected=0.999 arcsec robust_rms_after=0.978 arcsec worst_quadrant_rms_before=1.130 worst_quadrant_rms_after=1.106
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.130 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits N_match=4836 sigma_overall_arcsec=0.879 sigma_q1_arcsec=0.975 sigma_q2_arcsec=0.988 sigma_q3_arcsec=0.769 sigma_q4_arcsec=0.770 n_q1=1701 n_q2=1087 n_q3=1185 n_q4=863 worst_quadrant_to_overall_ratio=1.125
The image catalog is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits -region wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.nazXp8bpSd (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
WCS_IMAGE_NAME=wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
WCS-calibrated image found: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Checking if the catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat corresponding to the image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits alredy exist and is non-empty...
Catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat corresponding to the image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
WCS catalog name: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=150, bad_region=1, passed=5716
Got 5716 stars (including 5556 good ones) from the SExtractor catalog wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 5716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 4853 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 4843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 5712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 4854 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 5712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 5712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Excluding outliers - 4845 stars left (next iteration limit 5328)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4845 robust_rms=6.394 arcsec worst_quadrant_rms=23.284 arcsec
SIP_REFIT: SIP order 3 trial: matched=4845 robust_rms=1.078 arcsec worst_quadrant_rms=1.246 arcsec
SIP_REFIT: SIP order 5 trial: matched=4845 robust_rms=0.972 arcsec worst_quadrant_rms=1.116 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4845 robust_rms_before=1.387 arcsec robust_rms_before_corrected=1.000 arcsec robust_rms_after=0.972 arcsec worst_quadrant_rms_before=1.109 worst_quadrant_rms_after=1.116
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 1.109 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits N_match=4845 sigma_overall_arcsec=0.905 sigma_q1_arcsec=0.996 sigma_q2_arcsec=0.975 sigma_q3_arcsec=0.787 sigma_q4_arcsec=0.797 n_q1=1713 n_q2=1089 n_q3=1218 n_q4=825 worst_quadrant_to_overall_ratio=1.101
The image catalog is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits -region wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-06-44_20.00sec_0.00C_LIGHTs_0138.fits
Saving fully-calibrated image wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_PsA-04-Q1b1x1_000816_TTUQ1b1x1_968591_XNqRKm0i/wcs_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139.fits
Preparing the HTML report for the field PsA-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:32:53.33 -38:47:45.5: 12.36 +/- 0.14 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:34:07.98 -38:17:59.9: 11.84 +/- 0.09 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:34:55.91 -38:43:00.4: 12.44 +/- 0.16 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:31:41.12 -38:18:19.7: 12.21 +/- 0.12 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:31:01.70 -38:09:45.1: 12.54 +/- 0.16 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:34:44.85 -37:55:20.3: 12.14 +/- 0.12 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:39:38.85 -37:45:37.6: 13.06 +/- 0.20 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:32:35.24 -38:04:50.7: 12.56 +/- 0.16 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:44:28.23 -38:41:42.2: 12.91 +/- 0.19 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:34:07.98 -38:17:59.9: 11.89 +/- 0.08 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:32:35.24 -38:04:50.7: 12.86 +/- 0.18 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:32:53.33 -38:47:45.5: 12.82 +/- 0.18 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:34:44.85 -37:55:20.3: 12.61 +/- 0.15 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.06
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:34:55.91 -38:43:00.4: 13.04 +/- 0.22 detection
Forced photometry filter REJECTED candidate at 23:34:07.98 -38:17:59.9: ref_mag=11.87 +/- 0.06 new_mean_mag=11.5353 delta=0.34 (need > 0.90)
Forced photometry reference-image weighted average: 12.69 +/- 0.12
Forced photometry reference-image weighted average: 12.54 +/- 0.11
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:39:38.85 -37:45:37.6: 12.94 +/- 0.14 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.09
Forced photometry filter REJECTED candidate at 23:32:35.24 -38:04:50.7: ref_mag=12.69 +/- 0.12 new_mean_mag=12.0382 delta=0.65 (need > 0.90)
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:31:01.70 -38:09:45.1: 12.63 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 23:32:53.33 -38:47:45.5: ref_mag=12.54 +/- 0.11 new_mean_mag=12.0824 delta=0.45 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:34:44.85 -37:55:20.3: ref_mag=12.33 +/- 0.09 new_mean_mag=11.6144 delta=0.71 (need > 0.90)
Forced photometry reference-image weighted average: 12.65 +/- 0.13
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:31:41.12 -38:18:19.7: 12.49 +/- 0.13 detection
Forced photometry filter REJECTED candidate at 23:34:55.91 -38:43:00.4: ref_mag=12.65 +/- 0.13 new_mean_mag=11.7878 delta=0.86 (need > 0.90)
Forced photometry reference-image weighted average: 12.98 +/- 0.12
Forced photometry reference-image weighted average: 12.59 +/- 0.11
Forced photometry filter REJECTED candidate at 22:39:38.85 -37:45:37.6: ref_mag=12.98 +/- 0.12 new_mean_mag=12.1880 delta=0.79 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:31:01.70 -38:09:45.1: ref_mag=12.59 +/- 0.11 new_mean_mag=12.0313 delta=0.56 (need > 0.90)
Forced photometry reference-image weighted average: 12.35 +/- 0.09
Forced photometry filter REJECTED candidate at 23:31:41.12 -38:18:19.7: ref_mag=12.35 +/- 0.09 new_mean_mag=11.7925 delta=0.56 (need > 0.90)
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:44:28.23 -38:41:42.2: 13.15 +/- 0.19 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.13
Forced photometry filter REJECTED candidate at 22:44:28.23 -38:41:42.2: ref_mag=13.03 +/- 0.13 new_mean_mag=12.1832 delta=0.85 (need > 0.90)
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:25:49.47 -33:59:24.8: 13.26 +/- 0.24 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:25:21.40 -33:46:04.4: 13.03 +/- 0.19 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:22:23.77 -33:56:51.4: 13.34 +/- 0.29 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:33:13.05 -38:11:40.1: 12.66 +/- 0.19 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:33:16.99 -37:59:43.2: 12.71 +/- 0.19 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:25:20.42 -34:27:37.4: 12.88 +/- 0.18 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:23:47.63 -34:53:07.4: 11.21 +/- 0.04 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:23:08.87 -34:17:56.4: 12.37 +/- 0.12 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:33:13.05 -38:11:40.1: 12.97 +/- 0.19 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:25:49.47 -33:59:24.8: 13.10 +/- 0.16 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:25:21.40 -33:46:04.4: 13.45 +/- 0.23 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.13
Forced photometry reference-image weighted average: 13.15 +/- 0.13
Forced photometry filter REJECTED candidate at 23:33:13.05 -38:11:40.1: ref_mag=12.81 +/- 0.13 new_mean_mag=12.2624 delta=0.55 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:25:49.47 -33:59:24.8: ref_mag=13.15 +/- 0.13 new_mean_mag=12.4756 delta=0.68 (need > 0.90)
Forced photometry reference-image weighted average: 13.21 +/- 0.15
Forced photometry filter REJECTED candidate at 23:25:21.40 -33:46:04.4: ref_mag=13.21 +/- 0.15 new_mean_mag=12.5401 delta=0.67 (need > 0.90)
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:25:20.42 -34:27:37.4: 13.38 +/- 0.23 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:33:16.99 -37:59:43.2: 12.92 +/- 0.18 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.14
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:22:23.77 -33:56:51.4: 13.39 +/- 0.22 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.13
Forced photometry filter REJECTED candidate at 22:25:20.42 -34:27:37.4: ref_mag=13.08 +/- 0.14 new_mean_mag=12.3643 delta=0.71 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:33:16.99 -37:59:43.2: ref_mag=12.82 +/- 0.13 new_mean_mag=11.9550 delta=0.87 (need > 0.90)
Forced photometry reference-image weighted average: 13.38 +/- 0.17
Forced photometry filter KEPT candidate at 22:22:23.77 -33:56:51.4: ref_mag=13.38 +/- 0.17 new_mean_mag=12.3240 delta=1.05 (need > 0.90)
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:23:47.63 -34:53:07.4: 11.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.02
Forced photometry filter KEPT candidate at 22:23:47.63 -34:53:07.4: ref_mag=11.18 +/- 0.02 new_mean_mag=10.2048 delta=0.97 (need > 0.90)
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:23:08.87 -34:17:56.4: 12.48 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.08
Forced photometry filter KEPT candidate at 22:23:08.87 -34:17:56.4: ref_mag=12.43 +/- 0.08 new_mean_mag=11.4768 delta=0.96 (need > 0.90)
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 22:27:21.30 -34:11:21.8: 12.74 +/- 0.16 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-09_04-43-17_20.00sec_-0.00C_LIGHT_0207.fits at 23:08:27.97 -37:17:54.8: 12.97 +/- 0.19 detection
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 22:27:21.30 -34:11:21.8: 12.66 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.09
Forced photometry filter REJECTED candidate at 22:27:21.30 -34:11:21.8: ref_mag=12.68 +/- 0.09 new_mean_mag=11.8361 delta=0.85 (need > 0.90)
Forced photometry on wcs_PsA-04-Q1b1x1_2026-07-10_04-19-55_20.00sec_4.90C_LIGHT_0403.fits at 23:08:27.97 -37:17:54.8: 12.67 +/- 0.11 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.10
Forced photometry filter REJECTED candidate at 23:08:27.97 -37:17:54.8: ref_mag=12.75 +/- 0.10 new_mean_mag=11.9752 delta=0.77 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out22494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03848.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22285_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22285_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22361_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
Preparing report for the candidate 22361_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22391_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22391_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22392_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22392_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
**** FOUND 22:53:30.74 -32:55:41.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22405_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22405_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22411_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22411_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22430_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22430_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22436_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22436_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22439_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22439_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22448_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22448_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22450_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22450_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22452_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22452_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22487_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22487_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22494_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22494_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
**** FOUND 22:22:23.77 -33:56:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.166 6599718322664242688 335.59901245871 -33.94757202470 13.0434 12.5443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22495_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22495_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22510_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22510_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22511_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 22511_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04030_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 04030_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
**** FOUND 22:54:18.70 -34:23:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03279_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
Preparing report for the candidate 03279_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03848_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
Preparing report for the candidate 03848_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01836_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 01836_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
**** FOUND 22:47:50.08 -36:42:08.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20136_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 20136_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20009_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139
The candidate 20009_fd_PsA-04-Q1b1x1_2026-09-07_00-07-35_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks