This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL
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,2461149.7347,10.17,0.05,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 20260419.2347 10.17CV 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,2461149.7347,13.19,0.05,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 20260419.2347 13.19CV 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,2461149.7347,14.45,0.05,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 20260419.2347 14.45CV 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 19.2347* 11 25 50.21 -06 22 03.3 14.4 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,2461149.7347,14.43,0.05,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 20260419.2347 14.43CV 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: 2461149.73503749 19.04.2026 05:38:17.239 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
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: 6 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): 6600
Objects passed selection criteria: 6599
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 6192.25
Average stars matched: 6040.75 (97.5534 %)
Memory usage VmPeak: 112272 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 Sun Apr 19 00:41:42 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: 2461149.73503749 19.04.2026 05:38:17.239 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 59
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
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: 19 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): 40785
Objects passed selection criteria: 40682
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 38635.5
Average stars matched: 37066.8 (95.9396 %)
Memory usage VmPeak: 140128 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 Sun Apr 19 00:42:54 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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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: 2461149.73428477
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits exists and is non-empty
Saving wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits to local_wcs_cache/
'wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits' -> 'local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits'
wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits exists and is non-empty
Saving wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits to local_wcs_cache/
'wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits' -> 'local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits (1st new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
Image size: 941.4'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: 11:08:29.936 -10:00:18.36 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 11:08:29.936 -10:00:18.36
Angular distance between the image centers 0.0379 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits (2nd new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
Image size: 941.4'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: 11:08:33.015 -10:00:15.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:33.015 -10:00:15.56
Angular distance between the image centers 0.0502 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 11:08:29.936 -10:00:18.36
Second-epoch second image center 11:08:33.015 -10:00:15.56
Angular distance between the image centers 0.01266 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.T7HAd6DYsX
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.j99OSVBrDB
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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits &> /tmp/tmp.OJsDVnGE6W
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits &> /tmp/tmp.8iZCVhkBqZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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 4 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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
2.1 pix fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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
14.9 mag. fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
14.9 mag. fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
All-image limiting magnitude estimate: 14.9 (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.T7HAd6DYsX (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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/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.j99OSVBrDB (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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/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.OJsDVnGE6W (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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=424, passed=5878
Got 5878 stars (including 5446 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat
util/solve_plate_with_UCAC5 got 5878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
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(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
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(), 5819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits -region wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.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.8iZCVhkBqZ (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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=429, passed=5866
Got 5866 stars (including 5425 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat
util/solve_plate_with_UCAC5 got 5866 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
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(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5789 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 -4.2)
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(), 5788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5788 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_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits -region wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits'
Saving fully-calibrated image wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits'
Preparing the HTML report for the field Crt-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20350.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 20350_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
Preparing report for the candidate 20350_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20392_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 20392_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:48:48.80 -09:00:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20473_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 20473_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:01:18.14 -10:03:14.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04837_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 04837_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:01:55.13 -07:39:41.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
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 ####
11:30:16.80 -14:22:47.8
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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits exists and is non-empty
wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits (1st new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
Image size: 941.4'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: 11:08:29.936 -10:00:18.36 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 11:08:29.936 -10:00:18.36
Angular distance between the image centers 0.0379 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits (2nd new image)
verification OK: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
Image size: 941.4'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: 11:08:33.015 -10:00:15.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:21.189 -10:01:02.52
Second-epoch image center 11:08:33.015 -10:00:15.56
Angular distance between the image centers 0.0502 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 11:08:29.936 -10:00:18.36
Second-epoch second image center 11:08:33.015 -10:00:15.56
Angular distance between the image centers 0.01266 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.JRcKym3Pmk
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.3qZOZeO7pM
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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits &> /tmp/tmp.pqceXWSVoE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits &> /tmp/tmp.7lx1JaL1YB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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 56 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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
2.0 pix fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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
15.1 mag. fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
15.1 mag. fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.JRcKym3Pmk (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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/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.3qZOZeO7pM (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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/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.pqceXWSVoE (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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1438, passed=37435
Got 37435 stars (including 35940 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat
util/solve_plate_with_UCAC5 got 37435 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 36996 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 431 (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
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 36998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 36999 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits -region wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.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.7lx1JaL1YB (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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
WCS_IMAGE_NAME=wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
WCS-calibrated image found: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
Checking if the catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat corresponding to the image wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
WCS catalog name: wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1428, passed=37607
Got 37607 stars (including 36116 good ones) from the SExtractor catalog wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat
util/solve_plate_with_UCAC5 got 37607 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 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: 962 matched stars entering correct_measured_positions(), 37048 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 431 (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
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 37046 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 37047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits -region wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/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_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-37-12_20.00sec_-4.90C_LIGHTs_0380.fits
Saving fully-calibrated image wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.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_2026-04-19_CI_Crt-01-Q1b1x1_003921_TTUQ1b1x1_985332_stMYofGL/wcs_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381.fits
Preparing the HTML report for the field Crt-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54310.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53233_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53233_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:21:56.84 -06:46:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53239_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53239_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:18:12.92 -07:05:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53242_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53242_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:37:51.05 -13:37:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53243_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53243_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:39:20.99 -05:48:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.522 3593550277015241856 174.83760006758 -05.81039499565 14.0558 13.5266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53248_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53248_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:36:04.80 -08:39:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53249_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53249_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:29:13.68 -05:22:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53250_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53250_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:49:33.77 -08:36:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53281_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53281_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:30:16.80 -14:22:47.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53472_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53472_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:37:27.63 -11:41:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53528_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53528_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:12:44.73 -07:18:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53660_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
Preparing report for the candidate 53660_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
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Considering the candidate 53666_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53666_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:27:17.46 -10:54:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53735_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 53735_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:02:05.51 -05:57:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54013_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54013_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:53:59.80 -11:51:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54049_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54049_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:32:52.46 -11:50:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54066_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54066_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:22:26.50 -07:06:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54126_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54126_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:37:21.54 -12:02:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54201_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54201_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:24:58.26 -14:54:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54211_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54211_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:37:11.72 -14:23:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54234_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54234_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:51:06.01 -14:19:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54247_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
Preparing report for the candidate 54247_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
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Considering the candidate 54267_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54267_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:37:20.71 -07:26:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54280_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54280_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:36:50.89 -07:27:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 1.337 3592172696320756992 174.21194043484 -07.46380213416 14.7260 14.2538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54304_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54304_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:24:43.99 -09:19:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 2.765 3590705741650881152 171.18285941701 -09.31811093294 14.8050 14.1498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54310_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
Preparing report for the candidate 54310_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
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Considering the candidate 54333_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54333_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:42:15.92 -05:36:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54343_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54343_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:04:24.36 -05:18:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 3.106 3788010148318005760 166.10161159819 -05.31063346741 14.9541 14.3651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54352_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54352_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:29:14.70 -07:17:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54362_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54362_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:38:11.01 -14:31:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54397_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54397_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:38:28.30 -09:54:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.839 3587094155191896704 174.61739946078 -09.90678702421 14.8018 14.2626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54423_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54423_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:46:26.85 -10:27:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54428_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54428_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:34:20.82 -08:10:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 0.792 3592014297926733824 173.58685959042 -08.17271930871 14.6986 14.1754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54433_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54433_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:34:37.00 -13:34:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 1.684 3585155510034745088 173.65388772793 -13.57713103185 14.5417 13.9077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54446_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54446_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:39:36.99 -05:27:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54448_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54448_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:33:15.07 -11:22:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54449_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54449_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:34:10.68 -06:06:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54452_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54452_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:32:18.79 -12:02:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.239 3586224544574342016 173.07819919281 -12.04544328812 14.6882 14.2488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54456_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54456_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:56:45.56 -05:41:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 0.033 3764657341682462336 164.18983887047 -05.69346497766 14.6850 14.0474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54457_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54457_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:30:05.23 -13:43:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54461_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54461_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:39:39.56 -11:21:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54472_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54472_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:26:47.62 -08:22:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.023 3591291850067881472 171.69839316313 -08.36922774751 14.7519 14.2348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54473_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54473_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:23:28.43 -05:45:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.027 3785670009616765440 170.86857624242 -05.75462891902 14.7994 14.2889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54476_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54476_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 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 54478_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54478_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:27:15.38 -13:08:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54493_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54493_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:44:30.29 -06:45:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54505_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54505_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:36:25.18 -08:47:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54523_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54523_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:34:24.04 -09:52:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.741 3590094069588426112 173.60053126329 -09.87421262252 14.7266 14.2751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54526_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54526_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:31:47.84 -09:52:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54528_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54528_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:35:48.52 -09:04:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.595 3591699047327494016 173.95261472054 -09.07877429155 14.8906 14.3060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54530_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54530_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:39:19.08 -06:29:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 2.258 3593373363018356480 174.82910440500 -06.49129441192 14.8439 14.3210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54531_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54531_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:55:01.31 -13:57:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 0.735 3563893119815270144 163.75524842745 -13.95851444518 14.8089 14.2065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54539_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54539_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:45:32.77 -12:07:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.757 3757451486070910592 161.38632708509 -12.12651340335 14.8304 14.3227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54542_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54542_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 10:55:17.73 -13:18:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 0.516 3756177465627405056 163.82374094225 -13.30955148705 14.9405 14.4248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54544_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 54544_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:35:32.89 -09:04:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 0.466 3591709527047695488 173.88714056222 -09.06827949120 14.6520 14.0285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 36681_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 36681_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks
**** FOUND 11:01:55.14 -07:39:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24735_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381
The candidate 24735_fd_Crt-01-Q1b1x1_2026-04-19_00-38-17_20.00sec_-5.00C_LIGHTs_0381 did not pass the final checks