This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF
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 06.2346* 11 33 09.54 +05 06 18.5 11.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7346,11.52,0.05,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 20260406.2346 11.52CV 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 06.2346* 11 09 01.38 +04 01 36.1 11.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7346,11.39,0.05,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 20260406.2346 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 06.2346* 10 55 37.09 +02 55 28.4 12.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7346,12.39,0.05,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 20260406.2346 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 06.2346* 11 23 13.89 +05 48 57.4 12.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7346,12.86,0.05,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 20260406.2346 12.86CV 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
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 06.2346* 11 06 41.90 +01 56 34.3 13.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7346,13.03,0.05,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 20260406.2346 13.03CV 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 06.2346* 11 07 16.50 +10 10 04.9 13.2 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7346,13.21,0.05,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 20260406.2346 13.21CV 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 06.2346* 11 10 01.76 +08 28 39.2 13.7 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7346,13.65,0.05,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 20260406.2346 13.65CV 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 06.2346* 11 34 55.63 +08 48 29.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7346,14.63,0.05,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 20260406.2346 14.63CV 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: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
First image: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Last image: 2461136.73588844 06.04.2026 05:39:30.761 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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): 4747
Objects passed selection criteria: 4745
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 4516.25
Average stars matched: 4370.25 (96.7672 %)
Memory usage VmPeak: 111000 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:45:36 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: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
First image: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Last image: 2461136.73588844 06.04.2026 05:39:30.761 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 52
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.40
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: 13 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): 26011
Objects passed selection criteria: 25939
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 23687.8
Average stars matched: 22849.5 (96.4613 %)
Memory usage VmPeak: 130208 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:46:34 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.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: 2461136.73339839
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
Saving wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits to local_wcs_cache/
'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
Saving wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits to local_wcs_cache/
'wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits'
wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:48.062 +06:01:13.84
Angular distance between the image centers 0.1552 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:47.137 +06:00:40.19
Angular distance between the image centers 0.1500 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:48.062 +06:01:13.84
Second-epoch second image center 11:08:47.137 +06:00:40.19
Angular distance between the image centers 0.01010 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.jZlAuzo6ui
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.pHSfqFixQa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits &> /tmp/tmp.AKDLiDShk6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits &> /tmp/tmp.YaRbBvHZUw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
Found non-empty wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
The reference image (wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits) and catalog (wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat) found
'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat' -> 'wcsmag.cat'
Read 5629 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.0658 to 175.0329 deg, Dec +0.7091 to +11.2821 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 159.0658 to 175.0329 deg, Dec 0.7091 to 11.2821 deg
Loaded 3938 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): 3214 out of 3354 total matches.
Matched with Tycho-2 3354 out of 5629 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.832371
a=0.000000 b=1.000000 c=22.832371
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.1 pix Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
4.1 pix fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
2.5 pix fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
Limiting magnitude estimates:
15.2 mag. Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
15.2 mag. Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
14.5 mag. fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
15.0 mag. fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jZlAuzo6ui (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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=5629
Got 5629 stars (including 5225 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 5629 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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.pHSfqFixQa (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=431, passed=5671
Got 5671 stars (including 5234 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
util/solve_plate_with_UCAC5 got 5671 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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.AKDLiDShk6 (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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=652, passed=5102
Got 5102 stars (including 4449 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat
util/solve_plate_with_UCAC5 got 5102 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.7'
Seting catalog search parameters based on the expected field of view 936.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013010 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010408 (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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4826 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits -region wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.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.YaRbBvHZUw (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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=353, passed=5184
Got 5184 stars (including 4824 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat
util/solve_plate_with_UCAC5 got 5184 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5109 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits -region wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
Saving fully-calibrated image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits'
Preparing the HTML report for the field Leo-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20307.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 20305_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
Preparing report for the candidate 20305_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20307_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
Preparing report for the candidate 20307_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
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Considering the candidate 20352_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 20352_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 11:31:21.31 +06:30:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.769 3910330503374317184 172.83858564635 +06.50880009334 12.2466 11.6448 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20357_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 20357_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 11:32:08.88 +06:00:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.265 3909500238952299264 173.03664670998 +06.01460729379 12.2914 11.7135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.265#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: 8s
Prepared the HTML report for the field Leo-07-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 ####
11:33:09.54 +05:06:18.5
11:09:01.38 +04:01:36.1
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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Creating symlink local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits exists and is non-empty
wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:48.062 +06:01:13.84
Angular distance between the image centers 0.1552 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:47.137 +06:00:40.19
Angular distance between the image centers 0.1500 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:48.062 +06:01:13.84
Second-epoch second image center 11:08:47.137 +06:00:40.19
Angular distance between the image centers 0.01010 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.O4QJGj2tpj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.K9m3lY8pWE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits &> /tmp/tmp.PMsGbMQm0F
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits &> /tmp/tmp.nwonLTOsWF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
Found non-empty wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
The reference image (wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits) and catalog (wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat) found
'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat' -> 'wcsmag.cat'
Read 31032 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.0537 to 175.0351 deg, Dec +0.7036 to +11.2819 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 159.0537 to 175.0351 deg, Dec 0.7036 to 11.2819 deg
Loaded 3942 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): 3142 out of 3441 total matches.
Matched with Tycho-2 3441 out of 31032 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.714936
a=0.000000 b=1.000000 c=22.714936
From vast_summary.log: estimated ref. image limiting mag.: -7.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.0 pix Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
3.7 pix fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
2.2 pix fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
Limiting magnitude estimates:
15.3 mag. Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
15.3 mag. Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
14.8 mag. fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
15.2 mag. fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.2 (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.O4QJGj2tpj (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1190, passed=31016
Got 31016 stars (including 29781 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 31016 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 30730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 30733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 30732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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.K9m3lY8pWE (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1251, passed=31400
Got 31400 stars (including 30103 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
util/solve_plate_with_UCAC5 got 31400 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 31073 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 31074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 31074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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.PMsGbMQm0F (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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2750, passed=20248
Got 20248 stars (including 17490 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat
util/solve_plate_with_UCAC5 got 20248 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.7'
Seting catalog search parameters based on the expected field of view 936.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013010 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010408 (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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 18985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 18986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 18986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits -region wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.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.nwonLTOsWF (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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1056, passed=27571
Got 27571 stars (including 26471 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat
util/solve_plate_with_UCAC5 got 27571 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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 27307 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 27311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 27311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits -region wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Saving fully-calibrated image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-35-55_20.00sec_-4.90C_LIGHT_0182.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.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_2026-04-06_CI_Leo-07-Q2b1x1_004011_TTUQ2b1x1_31822_Kl49lDwF/wcs_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183.fits
Preparing the HTML report for the field Leo-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52520.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 5s
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Considering the candidate 51995_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 51995_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:45:34.93 +07:11:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.763 3865545715443742336 161.39531787666 +07.19165867531 13.4915 12.8325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51996_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 51996_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:49:24.36 +02:21:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.634 3809141731011175424 162.35132396308 +02.36126846652 13.4514 12.7352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51999_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 51999_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:45:34.15 +07:14:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.919 3865558050589815552 161.39280890721 +07.23761684097 13.4333 12.8758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52010_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52010_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:45:22.92 +03:51:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.680 3857544019572154496 161.34568732507 +03.85319423067 13.0522 12.5679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52017_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52017_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:44:32.93 +07:34:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.393 3865618386290340992 161.13717438258 +07.57138164921 13.0476 12.4751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52021_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52021_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:46:40.23 +04:21:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.066 3858007012751182208 161.66732951243 +04.35316588800 13.1786 12.6779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52027_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52027_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:49:21.81 +02:13:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.800 3809091428354207744 162.34079984098 +02.23139456472 13.0650 12.3598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52040_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52040_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:45:27.02 +05:16:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.683 3858395518312915968 161.36232453307 +05.26618943737 12.9331 12.4492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52045_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52045_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:45:31.39 +05:27:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.491 3858415897933687552 161.38010156362 +05.45339001290 12.8067 12.2760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52056_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52056_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:44:10.54 +07:33:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.045 3865628659852115840 161.04282037090 +07.55740895679 12.7183 12.2808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52063_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52063_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:46:30.31 +06:50:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.816 3865340038050004864 161.62607098426 +06.84164150116 12.8292 12.3127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52065_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52065_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:45:26.59 +04:57:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.573 3858245778573203584 161.36010431699 +04.95635039228 12.6148 11.9895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52087_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52087_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:44:42.59 +05:02:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.196 3858293882206937088 161.17696900261 +05.04955012562 12.3162 11.6834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52090_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52090_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 10:44:12.60 +07:40:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 0.943 3865634565431899008 161.05223976413 +07.67148232863 12.2880 11.6499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52191_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52191_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 11:33:09.53 +05:06:18.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52196_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52196_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
**** FOUND 11:09:01.37 +04:01:36.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52254_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
Preparing report for the candidate 52254_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
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Considering the candidate 52259_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
Preparing report for the candidate 52259_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
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Considering the candidate 52267_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183
The candidate 52267_fd_Leo-07-Q2b1x1_2026-04-06_00-39-30_20.00sec_-5.00C_LIGHT_0183 did not pass the final checks
