This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461191.9145,8.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260531.4145 8.32CV 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
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,2461191.9145,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260531.4145 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461191.9145,8.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260531.4145 8.30CV 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
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,2461191.9145,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260531.4145 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.60800240 23.12.2025 02:35:21.407 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
First image: 2461032.60800240 23.12.2025 02:35:21.407 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Last image: 2461191.91476505 31.05.2026 09:57:05.700 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4832
Objects passed selection criteria: 4803
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 3176.5
Average stars matched: 2991 (94.1602 %)
Memory usage VmPeak: 111056 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 31 05:13:59 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.60800240 23.12.2025 02:35:21.407 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
First image: 2461032.60800240 23.12.2025 02:35:21.407 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Last image: 2461191.91476505 31.05.2026 09:57:05.700 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.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.: -7.46
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: 10 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): 26613
Objects passed selection criteria: 26536
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 18554
Average stars matched: 17265 (93.0527 %)
Memory usage VmPeak: 129688 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 26 15:05:11 CDT 2026
VaST build number 1.0rc89-83-g49118af2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-26)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 31 05:15:38 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
SExtractor catalog cache: saved Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat to cache
SExtractor catalog cache: saved Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.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: 2461191.91416626
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits exists and is non-empty
Saving wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits to local_wcs_cache/
'wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits' -> 'local_wcs_cache/wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits'
wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits exists and is non-empty
Saving wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits to local_wcs_cache/
'wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits' -> 'local_wcs_cache/wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits'
wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits exists and is non-empty
Saving wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits to local_wcs_cache/
'wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits' -> 'local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits'
wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits exists and is non-empty
Saving wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits to local_wcs_cache/
'wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits' -> 'local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits (1st reference image)
verification OK: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Image size: 941.5'x627.0' 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: 23:59:54.531 -02:01:08.13 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-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits (1st new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
Image size: 938.8'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:01.319 -01:59:45.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:54.531 -02:01:08.13
Second-epoch image center 00:00:01.319 -01:59:45.01
Angular distance between the image centers 0.0365 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits (2nd new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
Image size: 938.8'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:04.398 -01:59:09.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:54.531 -02:01:08.13
Second-epoch image center 00:00:04.398 -01:59:09.89
Angular distance between the image centers 0.0526 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 00:00:01.319 -01:59:45.01
Second-epoch second image center 00:00:04.398 -01:59:09.89
Angular distance between the image centers 0.01611 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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits &> /tmp/tmp.Q7jy7sUeDg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits &> /tmp/tmp.H0mjd341dK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits &> /tmp/tmp.k0WpKGPHeN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits &> /tmp/tmp.uXC9m5Dr8a
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat
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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat
Found non-empty wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat
The reference image (wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits) and catalog (wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat) found
'wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat' -> 'wcsmag.cat'
Read 6067 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9989 deg, Dec -7.3208 to +3.2939 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 0.0003 to 359.9989 deg, Dec -7.3208 to 3.2939 deg
Loaded 160398 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): 3377 out of 3518 total matches.
Matched with Tycho-2 3518 out of 6067 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.910100
a=0.000000 b=1.000000 c=22.910100
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6067 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9989 deg, Dec -7.3208 to +3.2939 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 0.0003 to 359.9989 deg, Dec -7.3208 to 3.2939 deg
Loaded 160398 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): 3377 out of 3518 total matches.
Matched with Tycho-2 3518 out of 6067 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits:
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits (aperture=6.2)
Read 5991 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9988 deg, Dec -7.3337 to +3.2897 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 0.0003 to 359.9988 deg, Dec -7.3337 to 3.2897 deg
Loaded 160571 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): 3355 out of 3514 total matches.
Matched with Tycho-2 3514 out of 5991 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits:
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
2.1 pix Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
2.4 pix fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
2.3 pix fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
2.1 pix wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
2.1 pix wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Limiting magnitude estimates:
15.2 mag. Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
15.2 mag. Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
13.7 mag. fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
13.7 mag. fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.0 (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.Q7jy7sUeDg (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits' -> 'wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=423, passed=6067
Got 6067 stars (including 5634 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat
util/solve_plate_with_UCAC5 got 6067 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 352.0769 through 0 to 7.8992, gap 7.8992 to 352.0769
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0770 through 0 to 7.8996, gap 7.8996 to 352.0770
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits N_match=963 sigma_overall_arcsec=0.309 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.329 sigma_q3_arcsec=0.334 sigma_q4_arcsec=0.243 n_q1=224 n_q2=259 n_q3=222 n_q4=258 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits -region wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.H0mjd341dK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.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-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits' -> 'wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, passed=5991
Got 5991 stars (including 5551 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 5991 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 352.0704 through 0 to 7.8991, gap 7.8991 to 352.0704
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5885 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 352.0705 through 0 to 7.8995, gap 7.8995 to 352.0705
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits N_match=962 sigma_overall_arcsec=0.337 sigma_q1_arcsec=0.439 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.256 n_q1=220 n_q2=258 n_q3=223 n_q4=261 worst_quadrant_to_overall_ratio=1.305
The image catalog is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits -region wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.k0WpKGPHeN (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_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.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_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=183, passed=2247
Got 2247 stars (including 2064 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat
util/solve_plate_with_UCAC5 got 2247 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (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 352.1381 through 0 to 7.9489, gap 7.9489 to 352.1381
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 2182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1382 through 0 to 7.9497, gap 7.9497 to 352.1382
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 2184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 2184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits N_match=961 sigma_overall_arcsec=0.396 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.515 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.499 n_q1=259 n_q2=209 n_q3=268 n_q4=225 worst_quadrant_to_overall_ratio=1.300
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits -region wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uXC9m5Dr8a (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_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.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_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=188, passed=2243
Got 2243 stars (including 2055 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 2243 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (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 352.1691 through 0 to 7.9487, gap 7.9487 to 352.1691
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 2182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1690 through 0 to 7.9495, gap 7.9495 to 352.1690
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 2182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 2182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits N_match=962 sigma_overall_arcsec=0.397 sigma_q1_arcsec=0.355 sigma_q2_arcsec=0.476 sigma_q3_arcsec=0.390 sigma_q4_arcsec=0.494 n_q1=260 n_q2=205 n_q3=267 n_q4=230 worst_quadrant_to_overall_ratio=1.245
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits -region wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits sigma_overall=0.309 worst_q_ratio=1.107
ref2=Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits sigma_overall=0.337 worst_q_ratio=1.305
new1=fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits sigma_overall=0.396 worst_q_ratio=1.300
new2=fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits sigma_overall=0.397 worst_q_ratio=1.245
reference average sigma_overall=0.323 worst_q_ratio=1.206
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057_astrometric_residuals.png (963 matched stars from wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058_astrometric_residuals.png (962 matched stars from wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389_astrometric_residuals.png (961 matched stars from wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390_astrometric_residuals.png (962 matched stars from wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits'
Saving fully-calibrated image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits'
Preparing the HTML report for the field Psc-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20231_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
Preparing report for the candidate 20231_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20548_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
Preparing report for the candidate 20548_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Psc-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
SExtractor catalog cache: saved Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat to cache
SExtractor catalog cache: saved Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Creating symlink local_wcs_cache/wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits exists and is non-empty
wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits exists and is non-empty
wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits exists and is non-empty
wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits (1st reference image)
verification OK: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Image size: 941.5'x627.0' 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: 23:59:54.531 -02:01:08.13 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-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits (1st new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
Image size: 938.8'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:01.319 -01:59:45.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:54.531 -02:01:08.13
Second-epoch image center 00:00:01.319 -01:59:45.01
Angular distance between the image centers 0.0365 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits (2nd new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
Image size: 938.8'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:04.398 -01:59:09.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:54.531 -02:01:08.13
Second-epoch image center 00:00:04.398 -01:59:09.89
Angular distance between the image centers 0.0526 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 00:00:01.319 -01:59:45.01
Second-epoch second image center 00:00:04.398 -01:59:09.89
Angular distance between the image centers 0.01611 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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits &> /tmp/tmp.ezjS1cWAuX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits &> /tmp/tmp.kGVVrrZzfB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits &> /tmp/tmp.1pd6tl4s3p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits &> /tmp/tmp.E54kJ9xT2L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat
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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat
Found non-empty wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat
The reference image (wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits) and catalog (wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat) found
'wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat' -> 'wcsmag.cat'
Read 32031 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9991 deg, Dec -7.3224 to +3.3002 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 0.0003 to 359.9991 deg, Dec -7.3224 to 3.3002 deg
Loaded 160540 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): 3289 out of 3587 total matches.
Matched with Tycho-2 3587 out of 32031 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.796500
a=0.000000 b=1.000000 c=22.796500
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 32031 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9991 deg, Dec -7.3224 to +3.3002 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 0.0003 to 359.9991 deg, Dec -7.3224 to 3.3002 deg
Loaded 160540 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): 3289 out of 3587 total matches.
Matched with Tycho-2 3587 out of 32031 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits:
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits (aperture=4.9)
Read 32121 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0003 to 359.9992 deg, Dec -7.3341 to +3.2914 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 0.0003 to 359.9992 deg, Dec -7.3341 to 3.2914 deg
Loaded 160607 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): 3279 out of 3591 total matches.
Matched with Tycho-2 3591 out of 32121 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits:
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
2.0 pix Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
2.4 pix fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
2.3 pix fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
2.0 pix wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
2.0 pix wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Limiting magnitude estimates:
15.3 mag. Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
15.3 mag. Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
13.8 mag. fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
13.9 mag. fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.4 (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.ezjS1cWAuX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.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-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits' -> 'wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1283, passed=32021
Got 32021 stars (including 30693 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat
util/solve_plate_with_UCAC5 got 32021 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 352.0737 through 0 to 7.9287, gap 7.9287 to 352.0737
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 31504 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0738 through 0 to 7.9292, gap 7.9292 to 352.0738
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 31503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 31503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits N_match=962 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.328 sigma_q2_arcsec=0.288 sigma_q3_arcsec=0.290 sigma_q4_arcsec=0.231 n_q1=225 n_q2=253 n_q3=226 n_q4=258 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits -region wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kGVVrrZzfB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.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-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits' -> 'wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1325, passed=32107
Got 32107 stars (including 30723 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 32107 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 352.0631 through 0 to 7.9155, gap 7.9155 to 352.0631
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 31619 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 352.0632 through 0 to 7.9160, gap 7.9160 to 352.0632
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 31619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 31619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits N_match=961 sigma_overall_arcsec=0.323 sigma_q1_arcsec=0.428 sigma_q2_arcsec=0.334 sigma_q3_arcsec=0.298 sigma_q4_arcsec=0.249 n_q1=222 n_q2=253 n_q3=230 n_q4=256 worst_quadrant_to_overall_ratio=1.323
The image catalog is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits -region wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1pd6tl4s3p (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_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.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_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=387, passed=13279
Got 13279 stars (including 12882 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat
util/solve_plate_with_UCAC5 got 13279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (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 352.1011 through 0 to 7.9489, gap 7.9489 to 352.1011
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13014 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1009 through 0 to 7.9497, gap 7.9497 to 352.1009
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13011 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13011 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits N_match=960 sigma_overall_arcsec=0.393 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.482 sigma_q3_arcsec=0.363 sigma_q4_arcsec=0.505 n_q1=262 n_q2=203 n_q3=263 n_q4=232 worst_quadrant_to_overall_ratio=1.287
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits -region wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.E54kJ9xT2L (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_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.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_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=554, passed=13848
Got 13848 stars (including 13280 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 13848 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010431 (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 352.1114 through 0 to 7.9487, gap 7.9487 to 352.1114
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13581 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1113 through 0 to 7.9495, gap 7.9495 to 352.1113
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits N_match=960 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.349 sigma_q2_arcsec=0.486 sigma_q3_arcsec=0.371 sigma_q4_arcsec=0.484 n_q1=260 n_q2=203 n_q3=266 n_q4=231 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits -region wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits.cat.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-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.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_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-56-13_20.00sec_4.90C_LIGHT_0389.fits
Saving fully-calibrated image wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.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_2026-05-31_CI_Psc-08-Q2b1x1_051002_TTUQ2b1x1_628968_w4lbvGF1/wcs_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390.fits
Preparing the HTML report for the field Psc-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 00:05:10.77 -05:41:48.6: 12.40 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:54:52.09 +00:04:17.4: 12.72 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 00:10:44.13 +02:02:36.3: 13.04 +/- 0.03 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 00:14:21.59 -02:13:28.8: 12.66 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-35-21_20.00sec_-15.00C_LIGHT_0057.fits at 23:59:45.79 -05:52:35.1: 12.43 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:54:52.09 +00:04:17.4: 12.72 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 00:10:44.13 +02:02:36.3: 13.04 +/- 0.03 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 23:59:45.79 -05:52:35.1: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter REJECTED candidate at 23:54:52.09 +00:04:17.4: ref_mag=12.72 +/- 0.02 new_mean_mag=12.6082 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:10:44.13 +02:02:36.3: ref_mag=13.04 +/- 0.02 new_mean_mag=12.9805 delta=0.06 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 00:05:10.77 -05:41:48.6: 12.42 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 23:59:45.79 -05:52:35.1: ref_mag=12.43 +/- 0.01 new_mean_mag=12.3894 delta=0.04 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2025-12-22_20-36-19_20.00sec_-15.00C_LIGHT_0058.fits at 00:14:21.59 -02:13:28.8: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter REJECTED candidate at 00:14:21.59 -02:13:28.8: ref_mag=12.64 +/- 0.01 new_mean_mag=12.6251 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:05:10.77 -05:41:48.6: ref_mag=12.41 +/- 0.01 new_mean_mag=12.4190 delta=-0.01 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 51749_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
Preparing report for the candidate 51749_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
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Considering the candidate 52088_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
Preparing report for the candidate 52088_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
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Considering the candidate 52678_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
The candidate 52678_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390 did not pass the final checks
**** FOUND 23:42:00.67 +01:48:29.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53032_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
The candidate 53032_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53118_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
The candidate 53118_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53131_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
The candidate 53131_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53332_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
The candidate 53332_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53755_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
The candidate 53755_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54037_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390
The candidate 54037_fd_Psc-08-Q2b1x1_2026-05-31_04-57-05_20.00sec_4.90C_LIGHT_0390 did not pass the final checks