This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.7436,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.2436 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.7436,13.18,0.05,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 20260417.2436 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 17.2436* 11 26 43.30 -06 28 56.3 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.7436,14.26,0.05,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 20260417.2436 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.7436,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.2436 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
First image: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Last image: 2461147.74397178 17.04.2026 05:51:09.162 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6484
Objects passed selection criteria: 6481
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 6058
Average stars matched: 5922 (97.755 %)
Memory usage VmPeak: 112268 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 00:53:18 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
First image: 2461058.92000603 18.01.2026 10:04:38.521 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Last image: 2461147.74397178 17.04.2026 05:51:09.162 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 61
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
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: 11 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): 40027
Objects passed selection criteria: 39915
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 37671.5
Average stars matched: 36340.5 (96.4668 %)
Memory usage VmPeak: 139984 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 00:54:04 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
SExtractor catalog cache: saved Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat to cache
SExtractor catalog cache: saved Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.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/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.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: 2461147.74331227
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits exists and is non-empty
Saving wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits to local_wcs_cache/
'wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> 'local_wcs_cache/wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
Saving wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits to local_wcs_cache/
'wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> 'local_wcs_cache/wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits exists and is non-empty
Saving wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits to local_wcs_cache/
'wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits' -> 'local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits'
wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits exists and is non-empty
Saving wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits to local_wcs_cache/
'wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits' -> 'local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits (1st reference image)
verification OK: wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Image size: 941.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:21.189 -10:01:02.52 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits (1st new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
Image size: 941.3'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:36.709 -10:01:48.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:36.709 -10:01:48.28
Angular distance between the image centers 0.0649 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits (2nd new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
Image size: 941.3'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:36.907 -10:01:14.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:36.907 -10:01:14.35
Angular distance between the image centers 0.0646 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 11:08:36.709 -10:01:48.28
Second-epoch second image center 11:08:36.907 -10:01:14.35
Angular distance between the image centers 0.00946 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/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits &> /tmp/tmp.hk8UbFyAYK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.sn76TWgfxk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits &> /tmp/tmp.vOjW1dEZ4x
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits &> /tmp/tmp.9VvEjWROYi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
Found non-empty wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
The reference image (wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits) and catalog (wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat) found
'wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat' -> 'wcsmag.cat'
Read 6631 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.9881 to 175.1919 deg, Dec -15.3070 to -4.7038 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 158.9881 to 175.1919 deg, Dec -15.3070 to -4.7038 deg
Loaded 4601 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3732 out of 3905 total matches.
Matched with Tycho-2 3905 out of 6631 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.839875
a=0.000000 b=1.000000 c=22.839875
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.10
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.10
Magnitude calibration plot:
____ 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: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
2.0 pix Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
2.1 pix fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
2.1 pix fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
Limiting magnitude estimates:
15.1 mag. Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
15.1 mag. Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
14.8 mag. fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
14.8 mag. fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hk8UbFyAYK (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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> 'wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS-calibrated image found: wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Checking if the catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS catalog name: wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=466, passed=6631
Got 6631 stars (including 6155 good ones) from the SExtractor catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 6631 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits -region wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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.sn76TWgfxk (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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> 'wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=470, passed=6561
Got 6561 stars (including 6079 good ones) from the SExtractor catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 6561 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.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.vOjW1dEZ4x (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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=380, passed=5580
Got 5580 stars (including 5197 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat
util/solve_plate_with_UCAC5 got 5580 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits -region wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.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.9VvEjWROYi (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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=376, passed=5612
Got 5612 stars (including 5230 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat
util/solve_plate_with_UCAC5 got 5612 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 5569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 5568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 5568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits -region wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.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_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
Saving fully-calibrated image wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
Saving fully-calibrated image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits'
Saving fully-calibrated image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits'
Preparing the HTML report for the field Crt-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20342.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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20342_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
Preparing report for the candidate 20342_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20399_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 20399_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 10:48:48.83 -09:00:01.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04837_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 04837_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:01:55.13 -07:39:41.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Crt-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 ####
11:31:23.18 -14:34:57.5
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/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
SExtractor catalog cache: saved Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat to cache
SExtractor catalog cache: saved Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Creating symlink local_wcs_cache/wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.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_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits exists and is non-empty
wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits exists and is non-empty
wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits (1st reference image)
verification OK: wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Image size: 941.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:21.189 -10:01:02.52 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits (1st new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
Image size: 941.3'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:36.709 -10:01:48.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:36.709 -10:01:48.28
Angular distance between the image centers 0.0649 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits (2nd new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
Image size: 941.3'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:36.907 -10:01:14.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:36.907 -10:01:14.35
Angular distance between the image centers 0.0646 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 11:08:36.709 -10:01:48.28
Second-epoch second image center 11:08:36.907 -10:01:14.35
Angular distance between the image centers 0.00946 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/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits &> /tmp/tmp.FXZHYwyEky
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.GQ0l49aFFn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits &> /tmp/tmp.vId9QxSSfj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits &> /tmp/tmp.5HgUQvrKRs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
Found non-empty wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
The reference image (wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits) and catalog (wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat) found
'wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat' -> 'wcsmag.cat'
Read 40110 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 158.9737 to 175.2111 deg, Dec -15.3080 to -4.7013 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 158.9737 to 175.2111 deg, Dec -15.3080 to -4.7013 deg
Loaded 4615 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3663 out of 4023 total matches.
Matched with Tycho-2 4023 out of 40110 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.714876
a=0.000000 b=1.000000 c=22.714876
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
1.9 pix Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
2.0 pix fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
2.0 pix fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
Limiting magnitude estimates:
15.2 mag. Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
15.3 mag. Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
15.0 mag. fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
15.0 mag. fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.FXZHYwyEky (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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits' -> 'wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS-calibrated image found: wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Checking if the catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
WCS catalog name: wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1646, passed=40101
Got 40101 stars (including 38397 good ones) from the SExtractor catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 40101 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 39628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 39629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 39628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits -region wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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.GQ0l49aFFn (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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits' -> 'wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1596, passed=40499
Got 40499 stars (including 38842 good ones) from the SExtractor catalog wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 40499 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 40100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 40102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 40101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.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.vId9QxSSfj (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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1393, passed=35522
Got 35522 stars (including 34077 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat
util/solve_plate_with_UCAC5 got 35522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 35143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 35142 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 35142 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits -region wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.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.5HgUQvrKRs (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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1375, passed=35628
Got 35628 stars (including 34205 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat
util/solve_plate_with_UCAC5 got 35628 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 35284 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 35283 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 35284 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits -region wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.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_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/wcs_Crt-01-Q1b1x1_2026-01-18_04-04-38_20.00sec_-14.90C_LIGHT_0477.fits
Saving fully-calibrated image wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/wcs_Crt-01-Q1b1x1_2026-01-18_04-05-18_20.00sec_-15.00C_LIGHT_0478.fits
Saving fully-calibrated image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-50-12_20.00sec_-4.90C_LIGHTs_0139.fits
Saving fully-calibrated image wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.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_2026-04-17_CI_Crt-01-Q1b1x1_005207_TTUQ1b1x1_2419966_IzArsV2W/wcs_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140.fits
Preparing the HTML report for the field Crt-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54181.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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53244_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53244_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 10:37:51.01 -13:37:26.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53247_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53247_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:46.56 -08:47:53.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53248_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53248_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:14:59.82 -14:33:32.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53250_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53250_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:34:09.20 -09:42:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.066 3590104995985232384 173.53804642251 -09.71033817982 13.8654 13.4436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53251_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53251_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:29:13.78 -05:22:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53252_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53252_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:33:43.81 -05:22:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53253_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53253_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 10:49:33.79 -08:36:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53277_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53277_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:31:23.18 -14:34:57.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53348_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53348_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:57.35 -06:29:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53422_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53422_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:23.50 -05:27:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53429_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53429_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:34.08 -05:31:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53469_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53469_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:37:27.58 -11:41:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53529_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53529_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:12:44.73 -07:18:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53534_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53534_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:27.31 -05:25:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53590_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53590_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:00.54 -14:52:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53595_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53595_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:29.25 -05:44:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53652_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53652_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:38:39.86 -05:23:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53656_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
Preparing report for the candidate 53656_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
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Considering the candidate 53657_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53657_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:36.02 -05:29:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53697_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53697_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:35.94 -05:53:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53894_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53894_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 10:40:53.94 -12:11:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53942_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53942_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:38.29 -05:30:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53949_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53949_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:38:21.99 -09:41:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 1.783 3588612993067102464 174.59195127106 -09.69140453308 14.1591 13.6729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53950_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53950_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:35.79 -05:51:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53984_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 53984_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:01:09.01 -11:39:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54039_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54039_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:27.93 -05:42:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54051_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
Preparing report for the candidate 54051_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
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Considering the candidate 54078_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54078_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:32:52.37 -11:50:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54083_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54083_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:09:48.35 -11:55:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54107_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54107_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:13:10.88 -13:30:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54162_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54162_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 10:52:11.46 -04:44:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 2.182 3777020009906857984 163.04719141793 -04.74271193955 14.4860 13.9612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54181_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
Preparing report for the candidate 54181_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
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Considering the candidate 54193_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54193_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:38:42.62 -05:50:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54221_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54221_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:22:26.43 -07:06:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54245_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54245_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 10:44:39.51 -10:33:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)GAIADR2_OUTPUT=# 1.490 3760762326036018688 161.16426860399 -10.56188683764 14.7982 14.2620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54261_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54261_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:15:54.40 -15:04:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 0.531 3560011294014148096 168.97655515862 -15.08037850791 14.4698 13.9748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54270_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54270_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:36:09.02 -11:12:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54295_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54295_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:28:54.93 -07:39:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54298_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54298_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:29:14.74 -07:17:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54306_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54306_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:33:14.97 -11:22:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54325_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54325_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:19.74 -11:46:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 3.110 3585837310322867840 174.83303073726 -11.77751398812 14.8011 14.3406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54328_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54328_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:39:31.94 -07:20:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.214 3592538387016244864 174.88305644164 -07.33750278229 14.7905 14.2328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54330_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54330_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 10:41:45.19 -06:43:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.796 3776297841220809856 160.43814280897 -06.71944216810 14.9204 14.4705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54331_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54331_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:24:28.39 -10:22:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 0.396 3589866298882885376 171.11831181088 -10.38246930529 15.0760 14.3222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54341_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54341_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:30:41.03 -14:52:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54349_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54349_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 10:55:41.38 -05:34:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54352_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54352_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:16:55.72 -09:57:20.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)
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Considering the candidate 54354_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54354_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:20:45.21 -12:41:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.320 3565196075454379008 170.18831597840 -12.69701546553 14.8741 14.1832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54356_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54356_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 10:44:49.57 -05:16:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.910 3776927586505690368 161.20671255050 -05.27960352440 14.7383 14.1082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54362_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54362_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:34:10.68 -06:06:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.812 3593623433194195968 173.54405091504 -06.10306547792 14.8768 14.3374 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54373_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 54373_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 10:49:00.11 -07:11:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 1.131 3764105386845312512 162.25064268600 -07.19908869665 14.6615 14.0216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34351_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 34351_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:38:43.75 -07:05:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36681_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 36681_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:01:55.14 -07:39:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27235_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 27235_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks
**** FOUND 11:33:45.22 -05:22:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24735_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140
The candidate 24735_fd_Crt-01-Q1b1x1_2026-04-17_00-51-09_20.00sec_-5.00C_LIGHTs_0140 did not pass the final checks