This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2144* 10 04 45.45 +18 47 09.7 13.4 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,2461146.7144,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2144 13.43CV 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
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 16.2144* 10 29 38.85 +25 01 11.0 13.6 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,2461146.7144,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2144 13.59CV 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 16.2144* 10 12 49.24 +17 47 11.5 14.6 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,2461146.7144,14.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2144 14.55CV 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 16.2144* 09 56 53.21 +20 05 24.9 14.7 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,2461146.7144,14.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2144 14.66CV 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 16.2144* 10 15 47.95 +20 36 39.1 13.9 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,2461146.7144,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2144 13.86CV 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: 2461093.76950778 22.02.2026 06:27:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
First image: 2461093.76950778 22.02.2026 06:27:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Last image: 2461146.71463728 16.04.2026 05:08:54.661 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6854
Objects passed selection criteria: 6828
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 5288.75
Average stars matched: 4855.75 (91.8128 %)
Memory usage VmPeak: 112104 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 00:17:06 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: 2461093.76950778 22.02.2026 06:27:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
First image: 2461093.76950778 22.02.2026 06:27:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Last image: 2461146.71463728 16.04.2026 05:08:54.661 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 144
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 18 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 35208
Objects passed selection criteria: 35077
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 28138.2
Average stars matched: 25732 (91.4485 %)
Memory usage VmPeak: 133988 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 00:18:05 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.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/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.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: 2461146.71412759
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits'
wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits'
wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits'
wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Image size: 937.6'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:09:07.513 +22:03:31.11 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:23.057 +21:58:17.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:07.513 +22:03:31.11
Second-epoch image center 10:09:23.057 +21:58:17.13
Angular distance between the image centers 0.1059 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:23.126 +21:58:13.95 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:07.513 +22:03:31.11
Second-epoch image center 10:09:23.126 +21:58:13.95
Angular distance between the image centers 0.1068 deg.
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# 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 10:09:23.057 +21:58:17.13
Second-epoch second image center 10:09:23.126 +21:58:13.95
Angular distance between the image centers 0.00092 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00092 deg. (min. required shift: 0.00164 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/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.d7zZHXwIET
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits &> /tmp/tmp.aZAwlIzRIt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits &> /tmp/tmp.Om7CPhPfSG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits &> /tmp/tmp.P2O2Nk7SCM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.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_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.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_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
Found non-empty wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
The reference image (wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits) and catalog (wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat) found
'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat' -> 'wcsmag.cat'
Read 7416 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.6263 to 161.4713 deg, Dec +15.9835 to +27.7570 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 143.6263 to 161.4713 deg, Dec 15.9835 to 27.7570 deg
Loaded 5159 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): 3609 out of 3783 total matches.
Matched with Tycho-2 3783 out of 7416 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.939489
a=0.000000 b=1.000000 c=22.939489
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
2.4 pix Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
2.5 pix fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
2.5 pix fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
Limiting magnitude estimates:
15.4 mag. Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
15.4 mag. Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
15.2 mag. fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
15.2 mag. fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.3 (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.d7zZHXwIET (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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=459, passed=7416
Got 7416 stars (including 6953 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 7416 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 7279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 7278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 7278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 901 stars left (next iteration limit 991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.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.aZAwlIzRIt (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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits' -> 'wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=475, passed=7467
Got 7467 stars (including 6987 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 7467 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 7338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 7338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 7339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 898 stars left (next iteration limit 987)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits -region wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.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.Om7CPhPfSG (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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=399, passed=6535
Got 6535 stars (including 6133 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 6535 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 904 matched stars entering correct_measured_positions(), 895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 904 matched stars entering correct_measured_positions(), 6433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 6434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 6433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 903 stars left (next iteration limit 994)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits -region wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.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.P2O2Nk7SCM (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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=412, passed=6553
Got 6553 stars (including 6139 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 6553 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 6439 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 6438 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 6435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 901 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits -region wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.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_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits'
Saving fully-calibrated image wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits'
Preparing the HTML report for the field Leo-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21448.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 21448_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 21448_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 09:59:58.57 +21:14:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.417 629454429623625088 149.99400010127 +21.24989094562 12.6121 12.1594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Leo-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.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_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits exists and is non-empty
wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits exists and is non-empty
wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Image size: 937.6'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:09:07.513 +22:03:31.11 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:23.057 +21:58:17.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:07.513 +22:03:31.11
Second-epoch image center 10:09:23.057 +21:58:17.13
Angular distance between the image centers 0.1059 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:23.126 +21:58:13.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:07.513 +22:03:31.11
Second-epoch image center 10:09:23.126 +21:58:13.95
Angular distance between the image centers 0.1068 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 10:09:23.057 +21:58:17.13
Second-epoch second image center 10:09:23.126 +21:58:13.95
Angular distance between the image centers 0.00092 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00092 deg. (min. required shift: 0.00164 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/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.U4PyPQuXRp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits &> /tmp/tmp.u70yYXbsUg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits &> /tmp/tmp.9a7gVxGfoS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits &> /tmp/tmp.f22gLpa8Ty
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.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_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.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_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
Found non-empty wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
The reference image (wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits) and catalog (wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat) found
'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat' -> 'wcsmag.cat'
Read 36419 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.6171 to 161.4713 deg, Dec +15.9835 to +27.7791 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 143.6171 to 161.4713 deg, Dec 15.9835 to 27.7791 deg
Loaded 5179 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): 3446 out of 3795 total matches.
Matched with Tycho-2 3795 out of 36419 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.820111
a=0.000000 b=1.000000 c=22.820111
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 94 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
2.3 pix Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
2.2 pix fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
2.2 pix fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
Limiting magnitude estimates:
15.6 mag. Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
15.6 mag. Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
15.5 mag. fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
15.5 mag. fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.8 (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.U4PyPQuXRp (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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=1750, passed=36394
Got 36394 stars (including 34600 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 36394 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 35738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 35738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 35738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 897 stars left (next iteration limit 986)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.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.u70yYXbsUg (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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits' -> 'wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1825, passed=36174
Got 36174 stars (including 34311 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 36174 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 35506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 35506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 35507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 891 stars left (next iteration limit 981)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits -region wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.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.9a7gVxGfoS (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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=1467, passed=33957
Got 33957 stars (including 32432 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 33957 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 33325 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 33323 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 33323 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 900 stars left (next iteration limit 990)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits -region wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.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.f22gLpa8Ty (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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1487, passed=34004
Got 34004 stars (including 32467 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 34004 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 33298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 33297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 33297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 897 stars left (next iteration limit 986)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits -region wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.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_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Saving fully-calibrated image wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-10_20.00sec_-4.90C_LIGHT_0172.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.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_2026-04-16_CI_Leo-02-Q2b1x1_001246_TTUQ2b1x1_31617_5Jfdrog8/wcs_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173.fits
Preparing the HTML report for the field Leo-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out13809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56760.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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: 4s
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Considering the candidate 51986_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 51986_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 10:07:09.38 +17:46:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51987_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 51987_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 09:51:27.61 +24:23:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 2.079 643010828173659648 147.86560416380 +24.39873321085 14.7809 14.2194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52587_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 52587_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52901_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 52901_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53217_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 53217_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 09:51:32.69 +24:49:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53219_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 53219_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53336_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 53336_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53493_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 53493_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53565_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 53565_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53631_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 53631_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53907_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 53907_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53952_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 53952_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54096_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54096_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54203_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54203_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54239_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
Preparing report for the candidate 54239_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
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Considering the candidate 54307_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54307_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54372_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54372_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54447_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54447_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54491_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
Preparing report for the candidate 54491_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
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Considering the candidate 54512_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54512_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54577_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54577_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54578_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54578_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 10:00:00.47 +21:15:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54631_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54631_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54640_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54640_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54722_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54722_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54798_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54798_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54811_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54811_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54843_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54843_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54861_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54861_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54920_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54920_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54970_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54970_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54976_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 54976_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55033_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55033_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55095_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55095_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55142_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55142_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55146_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55146_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55167_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55167_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55171_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55171_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55350_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55350_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55535_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55535_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55593_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55593_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55635_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55635_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55646_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55646_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55721_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55721_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55724_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55724_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 10:09:35.31 +21:35:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55742_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55742_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55757_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55757_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55762_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55762_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55796_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55796_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55893_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55893_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55924_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55924_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 09:53:58.77 +25:45:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55963_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 55963_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56059_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56059_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 10:27:01.53 +24:56:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56061_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56061_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 09:52:37.90 +23:55:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56107_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56107_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56165_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56165_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56223_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56223_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56285_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56285_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56304_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56304_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56307_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56307_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56330_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56330_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56344_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56344_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 09:52:16.18 +19:05:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56350_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56350_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56423_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56423_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56427_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
Preparing report for the candidate 56427_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
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Considering the candidate 56437_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56437_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56444_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56444_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56523_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56523_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56561_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56561_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 09:51:05.85 +23:53:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56700_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56700_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56702_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56702_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 09:58:17.95 +24:02:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56724_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56724_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56760_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
Preparing report for the candidate 56760_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
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Considering the candidate 56771_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56771_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56777_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56777_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56907_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56907_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56918_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56918_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56946_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56946_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56994_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 56994_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57000_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57000_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57032_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57032_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 09:56:10.31 +20:40:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57119_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57119_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 10:13:45.21 +26:15:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57156_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57156_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57172_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57172_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57288_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57288_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57356_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57356_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 10:13:41.24 +26:11:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57519_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57519_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57791_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57791_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57809_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57809_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57859_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57859_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
**** FOUND 10:13:48.95 +22:55:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57878_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57878_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57908_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 57908_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 13809_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
Preparing report for the candidate 13809_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
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Considering the candidate 18350_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173
The candidate 18350_fd_Leo-02-Q2b1x1_2026-04-16_00-08-54_20.00sec_-4.90C_LIGHT_0173 did not pass the final checks