This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 17.4401 2461208.9401 13.21 23:35:07.15 +11:00:56.6
94.51710 -47.60128 galactic Peg Second-epoch detections are separated by 1.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.695 Bella -1 -0 1 13.6 -0 0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:35:07.15 +11:00:56.6: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 23:35:07.15 +11:00:56.6: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461208.9401,13.21,0.05,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
VARIABLE_NAME 20260617.4401 13.21CV 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 06 17.4401 2461208.9401 13.25 00:11:31.95 +09:49:53.3
106.91064 -51.79462 galactic Psc Second-epoch detections are separated by 1.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.165 Loreley -1 -0 1 13.6 0 0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:11:31.95 +09:49:53.3: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 00:11:31.95 +09:49:53.3: 15.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461208.9401,13.25,0.05,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 20260617.4401 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 17.4401 2461208.9401 13.72 23:32:01.36 +02:07:44.2
86.60986 -55.04199 galactic Psc Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.338 Budrosa -2 0 2 14.1 0 0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:32:01.36 +02:07:44.2: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 23:32:01.36 +02:07:44.2: 15.36 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461208.9401,13.72,0.05,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 20260617.4401 13.72CV 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: 2461061.61251426 21.01.2026 02:41:51.232 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
First image: 2461061.61251426 21.01.2026 02:41:51.232 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Last image: 2461208.94030127 17.06.2026 10:33:52.030 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.78
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5426
Objects passed selection criteria: 5416
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 4836.25
Average stars matched: 4730 (97.803 %)
Memory usage VmPeak: 111436 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jun 17 05:38:54 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: 2461061.61251426 21.01.2026 02:41:51.232 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
First image: 2461061.61251426 21.01.2026 02:41:51.232 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Last image: 2461208.94030127 17.06.2026 10:33:52.030 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 29549
Objects passed selection criteria: 29494
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: 24828.2
Average stars matched: 24057.8 (96.8967 %)
Memory usage VmPeak: 132816 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jun 17 05:40:40 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.cat to cache
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.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/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461208.93985007
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits exists and is non-empty
Saving wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits to local_wcs_cache/
'wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits' -> 'local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits'
wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits exists and is non-empty
Saving wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits to local_wcs_cache/
'wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits' -> 'local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits'
wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits exists and is non-empty
Saving wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits to local_wcs_cache/
'wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits' -> 'local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits'
wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits exists and is non-empty
Saving wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits to local_wcs_cache/
'wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits' -> 'local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits (1st reference image)
verification OK: wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Image size: 941.8'x627.1' 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: 00:00:08.246 +05:58:32.12 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits (1st new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:00.156 +06:02:54.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:08.246 +05:58:32.12
Second-epoch image center 00:00:00.156 +06:02:54.73
Angular distance between the image centers 0.0803 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits (2nd new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:02.596 +06:02:54.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:08.246 +05:58:32.12
Second-epoch image center 00:00:02.596 +06:02:54.47
Angular distance between the image centers 0.0765 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 00:00:00.156 +06:02:54.73
Second-epoch second image center 00:00:02.596 +06:02:54.47
Angular distance between the image centers 0.01011 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits &> /tmp/tmp.T4nI1hnx6t
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits &> /tmp/tmp.Tfwd9QkPIH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits &> /tmp/tmp.T75ZI0qGPn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits &> /tmp/tmp.cf0G2nQnIz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.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_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.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_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat
Found non-empty wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat
The reference image (wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits) and catalog (wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat) found
'wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat' -> 'wcsmag.cat'
Read 5657 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9997 deg, Dec +0.6890 to +11.2632 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 0.0001 to 359.9997 deg, Dec 0.6890 to 11.2632 deg
Loaded 178988 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): 3650 out of 3762 total matches.
Matched with Tycho-2 3762 out of 5657 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.804350
a=0.000000 b=1.000000 c=22.804350
From vast_summary.log: estimated ref. image limiting mag.: -7.78
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5657 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9997 deg, Dec +0.6890 to +11.2632 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 0.0001 to 359.9997 deg, Dec 0.6890 to 11.2632 deg
Loaded 178988 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): 3650 out of 3762 total matches.
Matched with Tycho-2 3762 out of 5657 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits:
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits (aperture=6.0)
Read 5616 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0007 to 359.9999 deg, Dec +0.6971 to +11.2717 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 0.0007 to 359.9999 deg, Dec 0.6971 to 11.2717 deg
Loaded 179019 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): 3652 out of 3766 total matches.
Matched with Tycho-2 3766 out of 5616 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits:
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
2.1 pix Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
3.5 pix fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
3.5 pix fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
2.1 pix wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
2.1 pix wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
Limiting magnitude estimates:
15.0 mag. Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
15.0 mag. Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
14.3 mag. fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
14.3 mag. fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.T4nI1hnx6t (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits' -> 'wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=353, passed=5657
Got 5657 stars (including 5296 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat
util/solve_plate_with_UCAC5 got 5657 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0600 through 0 to 8.0260, gap 8.0260 to 352.0600
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0599 through 0 to 8.0264, gap 8.0264 to 352.0599
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits N_match=976 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.310 sigma_q2_arcsec=0.292 sigma_q3_arcsec=0.292 sigma_q4_arcsec=0.264 n_q1=215 n_q2=272 n_q3=214 n_q4=275 worst_quadrant_to_overall_ratio=1.081
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits -region wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Tfwd9QkPIH (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits' -> 'wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=358, passed=5616
Got 5616 stars (including 5250 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat
util/solve_plate_with_UCAC5 got 5616 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0601 through 0 to 8.0220, gap 8.0220 to 352.0601
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0600 through 0 to 8.0224, gap 8.0224 to 352.0600
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5530 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5530 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits N_match=976 sigma_overall_arcsec=0.301 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.292 sigma_q3_arcsec=0.314 sigma_q4_arcsec=0.266 n_q1=214 n_q2=271 n_q3=219 n_q4=272 worst_quadrant_to_overall_ratio=1.163
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits -region wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.T75ZI0qGPn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=210, passed=4143
Got 4143 stars (including 3929 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat
util/solve_plate_with_UCAC5 got 4143 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9006 through 0 to 8.2039, gap 8.2039 to 351.9006
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 4088 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8999 through 0 to 8.2041, gap 8.2041 to 351.8999
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 4088 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 4088 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits N_match=973 sigma_overall_arcsec=0.333 sigma_q1_arcsec=0.372 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.283 sigma_q4_arcsec=0.342 n_q1=258 n_q2=215 n_q3=268 n_q4=232 worst_quadrant_to_overall_ratio=1.125
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits -region wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cf0G2nQnIz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=206, passed=4043
Got 4043 stars (including 3833 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat
util/solve_plate_with_UCAC5 got 4043 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9006 through 0 to 8.2039, gap 8.2039 to 351.9006
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 3998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8999 through 0 to 8.2041, gap 8.2041 to 351.8999
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 3998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 3998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits N_match=972 sigma_overall_arcsec=0.353 sigma_q1_arcsec=0.336 sigma_q2_arcsec=0.406 sigma_q3_arcsec=0.289 sigma_q4_arcsec=0.353 n_q1=259 n_q2=214 n_q3=268 n_q4=231 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits -region wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits sigma_overall=0.286 worst_q_ratio=1.081
ref2=Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits sigma_overall=0.301 worst_q_ratio=1.163
new1=fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits sigma_overall=0.333 worst_q_ratio=1.125
new2=fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits sigma_overall=0.353 worst_q_ratio=1.149
reference average sigma_overall=0.2935 worst_q_ratio=1.122
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080_astrometric_residuals.png (976 matched stars from wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081_astrometric_residuals.png (976 matched stars from wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276_astrometric_residuals.png (973 matched stars from wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277_astrometric_residuals.png (972 matched stars from wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits'
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits'
Preparing the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Psc-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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.cat to cache
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Creating symlink local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits exists and is non-empty
wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits (1st reference image)
verification OK: wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Image size: 941.8'x627.1' 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: 00:00:08.246 +05:58:32.12 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits (1st new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:00.156 +06:02:54.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:08.246 +05:58:32.12
Second-epoch image center 00:00:00.156 +06:02:54.73
Angular distance between the image centers 0.0803 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits (2nd new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:02.596 +06:02:54.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:08.246 +05:58:32.12
Second-epoch image center 00:00:02.596 +06:02:54.47
Angular distance between the image centers 0.0765 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 00:00:00.156 +06:02:54.73
Second-epoch second image center 00:00:02.596 +06:02:54.47
Angular distance between the image centers 0.01011 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits &> /tmp/tmp.netU106Zei
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits &> /tmp/tmp.HQvdbzDLxO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits &> /tmp/tmp.C23Dqv3I78
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits &> /tmp/tmp.3GU0kMlDHE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.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_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.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_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat
Found non-empty wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits and wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat
The reference image (wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits) and catalog (wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat) found
'wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat' -> 'wcsmag.cat'
Read 31418 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9997 deg, Dec +0.6886 to +11.2641 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 0.0001 to 359.9997 deg, Dec 0.6886 to 11.2641 deg
Loaded 179005 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): 3719 out of 3990 total matches.
Matched with Tycho-2 3990 out of 31418 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.693400
a=0.000000 b=1.000000 c=22.693400
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.14
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.14
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31418 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9997 deg, Dec +0.6886 to +11.2641 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 0.0001 to 359.9997 deg, Dec 0.6886 to 11.2641 deg
Loaded 179005 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): 3719 out of 3990 total matches.
Matched with Tycho-2 3990 out of 31418 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits:
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits (aperture=4.8)
Read 31537 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 359.9999 deg, Dec +0.6970 to +11.2729 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 0.0000 to 359.9999 deg, Dec 0.6970 to 11.2729 deg
Loaded 179047 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): 3708 out of 3989 total matches.
Matched with Tycho-2 3989 out of 31537 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits:
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
2.0 pix Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
3.3 pix fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
3.2 pix fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
2.0 pix wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
2.0 pix wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
Limiting magnitude estimates:
15.1 mag. Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
15.1 mag. Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
14.3 mag. fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
14.3 mag. fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.netU106Zei (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits' -> 'wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1105, passed=31412
Got 31412 stars (including 30248 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat
util/solve_plate_with_UCAC5 got 31412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0552 through 0 to 8.0260, gap 8.0260 to 352.0552
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 30996 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0551 through 0 to 8.0264, gap 8.0264 to 352.0551
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 30994 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 30994 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits N_match=973 sigma_overall_arcsec=0.292 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.298 sigma_q4_arcsec=0.262 n_q1=226 n_q2=265 n_q3=219 n_q4=263 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits -region wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.HQvdbzDLxO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits' -> 'wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1121, passed=31524
Got 31524 stars (including 30359 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat
util/solve_plate_with_UCAC5 got 31524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0465 through 0 to 8.0220, gap 8.0220 to 352.0465
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 31131 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0464 through 0 to 8.0224, gap 8.0224 to 352.0464
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 31133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 31133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits N_match=972 sigma_overall_arcsec=0.289 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.282 n_q1=226 n_q2=267 n_q3=219 n_q4=260 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits -region wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.C23Dqv3I78 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=893, passed=19046
Got 19046 stars (including 18131 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat
util/solve_plate_with_UCAC5 got 19046 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8713 through 0 to 8.2373, gap 8.2373 to 351.8713
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 18783 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8708 through 0 to 8.2375, gap 8.2375 to 351.8708
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 18785 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 18786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits N_match=971 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.377 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.282 sigma_q4_arcsec=0.321 n_q1=258 n_q2=205 n_q3=267 n_q4=241 worst_quadrant_to_overall_ratio=1.109
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits -region wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3GU0kMlDHE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=544, passed=18302
Got 18302 stars (including 17737 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat
util/solve_plate_with_UCAC5 got 18302 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8915 through 0 to 8.2373, gap 8.2373 to 351.8915
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 18057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8910 through 0 to 8.2375, gap 8.2375 to 351.8910
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 18057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 18057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits N_match=971 sigma_overall_arcsec=0.348 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.412 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.328 n_q1=255 n_q2=206 n_q3=270 n_q4=240 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits -region wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-13_20.00sec_0.00C_LIGHTs_0276.fits
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Psc-04-Q1b1x1_053432_TTUQ1b1x1_3317747_ZxnGsI8B/wcs_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277.fits
Preparing the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:30:08.19 +04:52:54.2: 12.16 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:35:07.15 +11:00:56.6: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:23:05.95 +03:13:57.8: 13.58 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:02:24.46 +08:23:06.8: 13.22 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:54:26.03 +09:08:59.0: 13.76 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:11:36.75 +04:46:42.6: 13.37 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:08:31.08 +06:36:47.9: 13.27 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:11:31.95 +09:49:53.3: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 23:32:01.36 +02:07:44.2: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 00:23:05.95 +03:13:57.8: 13.55 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 00:30:08.19 +04:52:54.2: 12.17 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 23:54:26.03 +09:08:59.0: 13.77 +/- 0.06 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-41-51_20.00sec_-15.00C_LIGHT_0080.fits at 00:30:48.82 +07:25:40.6: 13.30 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 00:11:36.75 +04:46:42.6: 13.34 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 00:11:31.95 +09:49:53.3: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 00:08:31.08 +06:36:47.9: 13.35 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 00:02:24.46 +08:23:06.8: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 23:35:07.15 +11:00:56.6: 15.47 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter REJECTED candidate at 00:23:05.95 +03:13:57.8: ref_mag=13.56 +/- 0.04 new_mean_mag=13.7575 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter REJECTED candidate at 00:30:08.19 +04:52:54.2: ref_mag=12.16 +/- 0.01 new_mean_mag=12.1580 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:54:26.03 +09:08:59.0: ref_mag=13.76 +/- 0.04 new_mean_mag=13.5275 delta=0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:11:36.75 +04:46:42.6: ref_mag=13.35 +/- 0.03 new_mean_mag=13.2987 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter REJECTED candidate at 00:08:31.08 +06:36:47.9: ref_mag=13.31 +/- 0.03 new_mean_mag=13.2830 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:02:24.46 +08:23:06.8: ref_mag=13.20 +/- 0.03 new_mean_mag=13.0892 delta=0.11 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 23:32:01.36 +02:07:44.2: 15.36 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-01-20_20-42-40_20.00sec_-15.00C_LIGHT_0081.fits at 00:30:48.82 +07:25:40.6: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry filter REJECTED candidate at 00:30:48.82 +07:25:40.6: ref_mag=13.31 +/- 0.03 new_mean_mag=12.9592 delta=0.35 (need > 0.90)
Adding exclusion_list_local.txt__out52645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52931.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52313_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
The candidate 52313_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52381_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
The candidate 52381_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 23:45:12.83 +08:14:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52466_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
The candidate 52466_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
**** FOUND 23:51:22.76 +09:20:48.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52477_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
The candidate 52477_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52626_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
The candidate 52626_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52645_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 52645_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52658_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 52658_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52688_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
The candidate 52688_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52693_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
The candidate 52693_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52749_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
The candidate 52749_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52931_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
Preparing report for the candidate 52931_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11720_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
The candidate 11720_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14939_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277
The candidate 14939_fd_Psc-04-Q1b1x1_2026-06-17_05-33-52_20.00sec_-0.00C_LIGHTs_0277 did not pass the final checks