This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN
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!
TCP 2026 02 12.1391* 01 33 51.59 +30 39 34.2 12.1 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 303379863975508224,2461083.6391,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 303379863975508224 20260212.1391 12.09CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:33:51.59 +30:39:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20_00sec_-15_00C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20_00sec_-14_90C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20_00sec_-15_00C_LIGHT_0084_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20_00sec_-14_90C_LIGHT_0083_fits__*pix.png animation_v2.gif
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.6391,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.1391 13.39CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:20:43.84 +27:05:35.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20_00sec_-15_00C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20_00sec_-14_90C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20_00sec_-15_00C_LIGHT_0084_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20_00sec_-14_90C_LIGHT_0083_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.1391* 01 31 38.30 +29 27 52.4 14.1 U Tri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.6391,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.1391 14.13CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:31:38.30 +29:27:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20_00sec_-15_00C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20_00sec_-14_90C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20_00sec_-15_00C_LIGHT_0084_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20_00sec_-14_90C_LIGHT_0180_fits__*pix.png resample_wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20_00sec_-14_90C_LIGHT_0083_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.68918611 23.12.2025 04:32:15.680 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
First image: 2461032.68918611 23.12.2025 04:32:15.680 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
Last image: 2461083.63933520 12.02.2026 03:20:28.561 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.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.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 11581
Objects passed selection criteria: 11562
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 10568.8
Average stars matched: 10410 (98.4979 %)
Memory usage VmPeak: 117164 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 21:26:15 CST 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: 2461032.68918611 23.12.2025 04:32:15.680 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
First image: 2461032.68918611 23.12.2025 04:32:15.680 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
Last image: 2461083.63933520 12.02.2026 03:20:28.561 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 59
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 18 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): 64558
Objects passed selection criteria: 64440
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 61465.8
Average stars matched: 59969.2 (97.5653 %)
Memory usage VmPeak: 166660 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 21:27:28 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
SExtractor catalog cache: saved Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat to cache
SExtractor catalog cache: saved Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.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: 2461083.63887275
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits exists and is non-empty
Saving wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits to local_wcs_cache/
'wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits' -> 'local_wcs_cache/wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits'
wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits exists and is non-empty
Saving wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits to local_wcs_cache/
'wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits' -> 'local_wcs_cache/wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits'
wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits exists and is non-empty
Saving wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits to local_wcs_cache/
'wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits' -> 'local_wcs_cache/wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits'
wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits exists and is non-empty
Saving wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits to local_wcs_cache/
'wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits' -> 'local_wcs_cache/wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:00:01.048 +29:59:44.04
Second-epoch image center 00:59:59.327 +29:59:56.73
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:00:01.048 +29:59:44.04
Second-epoch image center 00:59:57.288 +29:59:49.43
Angular distance between the image centers 0.01 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 00:59:59.327 +29:59:56.73
Second-epoch second image center 00:59:57.288 +29:59:49.43
Angular distance between the image centers 0.00763 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-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits &> /tmp/tmp.h6pCJpjyIC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits &> /tmp/tmp.ZjlEMHeVVP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits &> /tmp/tmp.bCeQxSCd9W
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits &> /tmp/tmp.Pqz2CY2Jz1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.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-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat
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-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat
Found non-empty wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat
The reference image (wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits) and catalog (wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat) found
'wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 6509 out of 12178 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.918247
a=0.000000 b=1.000000 c=22.918247
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
2.1 pix Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
2.0 pix fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
2.0 pix fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
Limiting magnitude estimates:
15.4 mag. Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
15.4 mag. Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
15.0 mag. fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
15.0 mag. fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.h6pCJpjyIC (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.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-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits' -> 'wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
WCS-calibrated image found: wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
Checking if the catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
WCS catalog name: wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=849, passed=12178
Got 12178 stars (including 11320 good ones) from the SExtractor catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat
util/solve_plate_with_UCAC5 got 12178 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
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits -region wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.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.ZjlEMHeVVP (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits' -> 'wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Checking if the catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS catalog name: wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=849, passed=12201
Got 12201 stars (including 11339 good ones) from the SExtractor catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
util/solve_plate_with_UCAC5 got 12201 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits -region wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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.bCeQxSCd9W (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_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.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_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
Checking if the catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
WCS catalog name: wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=615, passed=9059
Got 9059 stars (including 8435 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat
util/solve_plate_with_UCAC5 got 9059 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits -region wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.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.Pqz2CY2Jz1 (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_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.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_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
Checking if the catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
WCS catalog name: wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=620, passed=9048
Got 9048 stars (including 8413 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat
util/solve_plate_with_UCAC5 got 9048 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits -region wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits'
Saving fully-calibrated image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits'
Preparing the HTML report for the field Psc-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20625.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20618_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 20618_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:47:18.92 +32:41:06.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20625_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
Preparing report for the candidate 20625_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01266_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 01266_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:51:23.27 +34:22:33.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Psc-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
01:33:51.59 +30:39:34.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
SExtractor catalog cache: saved Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat to cache
SExtractor catalog cache: saved Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
Creating symlink local_wcs_cache/wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits exists and is non-empty
wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits exists and is non-empty
wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits exists and is non-empty
wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:00:01.048 +29:59:44.04
Second-epoch image center 00:59:59.327 +29:59:56.73
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:00:01.048 +29:59:44.04
Second-epoch image center 00:59:57.288 +29:59:49.43
Angular distance between the image centers 0.01 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 00:59:59.327 +29:59:56.73
Second-epoch second image center 00:59:57.288 +29:59:49.43
Angular distance between the image centers 0.00763 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-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits &> /tmp/tmp.aw0jiNHvwt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits &> /tmp/tmp.CRou97gSL7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits &> /tmp/tmp.G4fkWPg5Wv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits &> /tmp/tmp.TJp0wtUMdo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.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-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat
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-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat
Found non-empty wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits and wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat
The reference image (wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits) and catalog (wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat) found
'wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 6588 out of 67874 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.812273
a=0.000000 b=1.000000 c=22.812273
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 47 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
2.0 pix Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
1.9 pix fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
1.9 pix fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
Limiting magnitude estimates:
15.5 mag. Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
15.5 mag. Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
15.2 mag. fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
15.2 mag. fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.5 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.aw0jiNHvwt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.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-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits' -> 'wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
WCS-calibrated image found: wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
Checking if the catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits
WCS catalog name: wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=4195, passed=67850
Got 67850 stars (including 63551 good ones) from the SExtractor catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat
util/solve_plate_with_UCAC5 got 67850 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
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits -region wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-32-15_20.00sec_-14.90C_LIGHT_0180.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.CRou97gSL7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits' -> 'wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS_IMAGE_NAME=wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS-calibrated image found: wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
Checking if the catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits alredy exist and is non-empty...
Catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat corresponding to the image wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits
WCS catalog name: wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=4197, passed=67402
Got 67402 stars (including 63079 good ones) from the SExtractor catalog wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat
util/solve_plate_with_UCAC5 got 67402 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits -region wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-01-Q1b1x1_2025-12-22_22-33-20_20.00sec_-14.90C_LIGHT_0181.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.G4fkWPg5Wv (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_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.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_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
Checking if the catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
WCS catalog name: wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=2859, passed=56322
Got 56322 stars (including 53366 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat
util/solve_plate_with_UCAC5 got 56322 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits -region wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.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.TJp0wtUMdo (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_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.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_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
WCS_IMAGE_NAME=wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
WCS-calibrated image found: wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
Checking if the catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat corresponding to the image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
WCS catalog name: wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2730, passed=55675
Got 55675 stars (including 52844 good ones) from the SExtractor catalog wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat
util/solve_plate_with_UCAC5 got 55675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits -region wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.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_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-19-48_20.00sec_-14.90C_LIGHT_0083.fits
Saving fully-calibrated image wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.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_2026-02-11_CI_Psc-01-Q1b1x1_212221_TTUQ1b1x1_31466_zLqrxnsN/wcs_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084.fits
Preparing the HTML report for the field Psc-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out82451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out82816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out82528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82605.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 82451_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82451_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:58:57.16 +28:33:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.521 310923441451235584 014.73776907476 +28.55962665456 14.5903 14.3272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82462_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82462_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:32:50.11 +33:48:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82464_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82464_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:39:40.23 +32:18:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82467_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82467_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:25:48.84 +30:13:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82474_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82474_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:27:16.23 +28:59:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82475_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82475_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:33:26.45 +25:24:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82485_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82485_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:33:08.49 +33:25:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82522_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82522_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:15:54.78 +30:07:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82528_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
Preparing report for the candidate 82528_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
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Considering the candidate 82533_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82533_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:12:56.58 +30:05:41.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82553_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82553_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:09:15.35 +30:11:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.750 310004662047279360 017.31340392509 +30.19944584499 13.7074 13.1831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82557_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82557_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:37:57.42 +25:10:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82569_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82569_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:12:55.18 +26:00:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82599_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82599_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:33:35.43 +27:31:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82603_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82603_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:19:54.99 +27:43:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82605_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
Preparing report for the candidate 82605_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
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Considering the candidate 82609_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82609_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:32:19.30 +31:45:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.610 2859715467651208320 008.08094304175 +31.76115360923 14.1291 13.4589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82612_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82612_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:15:04.67 +33:20:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.438 314023720644578176 018.76949211387 +33.34965940924 14.6668 14.2237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82615_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82615_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:28:43.90 +26:24:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82618_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82618_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:42:42.11 +31:50:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 2.580 360691907569783424 010.67551551127 +31.84146508053 14.1943 13.5292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82627_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82627_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:53:33.11 +33:29:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.653 362633301506905472 013.38759217293 +33.48693499822 14.2197 13.6854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82635_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82635_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:16:13.57 +25:46:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.687 294734159228860672 019.05706170752 +25.77415375099 14.3844 13.8436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82639_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82639_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:57:27.02 +27:20:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82649_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82649_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:32:38.78 +29:38:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82665_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82665_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:59:31.83 +32:45:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 2.421 314464899685003008 014.88196558968 +32.75898066011 14.4443 13.8384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82682_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82682_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:20:50.57 +33:41:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.201 319820071068046464 020.21095080329 +33.69312329827 14.6137 14.0547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82683_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82683_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:53:17.19 +33:00:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.777 361104155710679552 013.32151903913 +33.01523660393 14.0635 13.3592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82685_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82685_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:52:20.33 +27:59:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82687_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82687_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:04:35.37 +29:38:38.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82711_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82711_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:26:43.86 +28:32:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.622 297035956757349248 021.68237701431 +28.54144075775 14.6510 14.1743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82720_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82720_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:20:04.24 +29:31:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82727_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82727_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:59:10.70 +27:50:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82746_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82746_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:07:25.45 +24:50:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.805 306251753983612032 016.85519968130 +24.84620880937 14.4161 13.9338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82750_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82750_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:42:20.63 +29:19:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 2.078 2810199202012407936 010.58587898475 +29.31781593459 14.3051 13.8088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82781_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82781_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:30:16.24 +28:32:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 3.715 296813855408496384 022.56649622504 +28.54136642338 14.7506 14.1551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82789_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82789_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:51:48.21 +30:36:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.956 312339681147424384 012.95103684242 +30.61311362482 14.6877 14.1763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82791_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82791_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:54:49.32 +29:11:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.054 311247866100880640 013.70554342836 +29.18665409323 14.6553 13.8798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82793_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82793_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:21:10.47 +30:33:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.572 309479301647555584 020.29351148441 +30.56618015425 14.2965 13.6268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82799_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82799_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:39:32.34 +31:19:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82806_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82806_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 01:31:38.98 +30:43:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 3.767 315302280868814848 022.91120731772 +30.72437014818 14.6829 14.1499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82813_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82813_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:46:17.51 +29:51:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 2.893 312232994159508224 011.57212575024 +29.86193609342 14.5996 14.0864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82816_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 82816_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:50:57.45 +33:17:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.050 361302136523241984 012.73953694169 +33.29961954206 14.5679 14.0243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 17342_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 17342_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 06437_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 06437_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:51:23.27 +34:22:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16018_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 16018_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 18699_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 18699_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks
**** FOUND 00:47:18.92 +32:41:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78100_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084
The candidate 78100_fd_Psc-01-Q1b1x1_2026-02-11_21-20-28_20.00sec_-15.00C_LIGHT_0084 did not pass the final checks