This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2228* 11 12 20.31 +01 33 22.1 12.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7228,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2228 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2228* 11 02 20.71 +02 52 42.7 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7228,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2228 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2228* 11 02 44.47 -01 31 08.4 13.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7228,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2228 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2228* 10 40 02.78 +00 22 13.8 13.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7228,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2228 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2228* 10 43 07.93 -04 32 03.0 14.3 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7228,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2228 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2228* 11 27 12.35 -06 32 32.3 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7228,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2228 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2228* 11 27 23.14 +01 49 03.6 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7228,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2228 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461146.72457155 16.04.2026 05:23:12.982 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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): 6594
Objects passed selection criteria: 6588
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: 6235.5
Average stars matched: 6044.5 (96.9369 %)
Memory usage VmPeak: 112200 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 01:13:37 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461146.72457155 16.04.2026 05:23:12.982 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 79
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
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: 12 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): 35343
Objects passed selection criteria: 35270
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: 33529.2
Average stars matched: 32039.5 (95.5569 %)
Memory usage VmPeak: 136380 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 01:14:21 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461146.72110780
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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
Saving wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits to local_wcs_cache/
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
Saving wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits to local_wcs_cache/
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits'
wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits (1st reference image)
verification OK: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Image size: 941.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:34.742 -01:59:53.74 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits (1st new image)
verification OK: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:41.605 -02:00:02.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:41.605 -02:00:02.74
Angular distance between the image centers 0.0287 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits (2nd new image)
verification OK: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:40.241 -02:00:52.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:40.241 -02:00:52.24
Angular distance between the image centers 0.0281 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 11:08:41.605 -02:00:02.74
Second-epoch second image center 11:08:40.241 -02:00:52.24
Angular distance between the image centers 0.01488 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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.qWkwxX4R44
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.kgqgL4IyqE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits &> /tmp/tmp.KhBSndLY2r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits &> /tmp/tmp.scnucrkm0f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat' -> 'wcsmag.cat'
Read 6399 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.2436 to 175.0501 deg, Dec -7.2952 to +3.3133 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 159.2436 to 175.0501 deg, Dec -7.2952 to 3.3133 deg
Loaded 3835 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): 3238 out of 3372 total matches.
Matched with Tycho-2 3372 out of 6399 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.879752
a=0.000000 b=1.000000 c=22.879752
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.5 pix fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
2.2 pix fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Limiting magnitude estimates:
15.2 mag. Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.2 mag. Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
15.0 mag. fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
15.2 mag. fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (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.qWkwxX4R44 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=432, passed=6399
Got 6399 stars (including 5960 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 6399 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 413 to 468 (Dec -7.3 to 3.3)
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...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 6330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 6329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 6329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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.kgqgL4IyqE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=407, passed=6519
Got 6519 stars (including 6107 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 6519 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 6416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 6418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 6418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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.KhBSndLY2r (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=397, passed=6097
Got 6097 stars (including 5689 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat
util/solve_plate_with_UCAC5 got 6097 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
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...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.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.scnucrkm0f (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=479, passed=6134
Got 6134 stars (including 5651 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat
util/solve_plate_with_UCAC5 got 6134 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
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...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 6072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 6072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 6072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
Saving fully-calibrated image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits'
Preparing the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20536_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 20536_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:00:24.15 -02:42:26.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Creating symlink local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits exists and is non-empty
wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits (1st reference image)
verification OK: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Image size: 941.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:34.742 -01:59:53.74 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits (1st new image)
verification OK: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:41.605 -02:00:02.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:41.605 -02:00:02.74
Angular distance between the image centers 0.0287 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits (2nd new image)
verification OK: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:40.241 -02:00:52.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:40.241 -02:00:52.24
Angular distance between the image centers 0.0281 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 11:08:41.605 -02:00:02.74
Second-epoch second image center 11:08:40.241 -02:00:52.24
Angular distance between the image centers 0.01488 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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.qVXi7xZRt6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.dyjhv9b9B0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits &> /tmp/tmp.71kH98nwRJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits &> /tmp/tmp.rs0XvXMTso
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat' -> 'wcsmag.cat'
Read 34371 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.2400 to 175.0938 deg, Dec -7.3026 to +3.3144 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 159.2400 to 175.0938 deg, Dec -7.3026 to 3.3144 deg
Loaded 3852 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): 3086 out of 3398 total matches.
Matched with Tycho-2 3398 out of 34371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774901
a=0.000000 b=1.000000 c=22.774901
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 64 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.4 pix fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
2.0 pix fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Limiting magnitude estimates:
15.3 mag. Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.3 mag. Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
15.2 mag. fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
15.4 mag. fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.6 (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.qVXi7xZRt6 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1404, passed=34365
Got 34365 stars (including 32904 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 34365 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 413 to 468 (Dec -7.3 to 3.3)
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...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 33882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 33882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 33882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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.dyjhv9b9B0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1420, passed=33111
Got 33111 stars (including 31640 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 33111 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 413 to 468 (Dec -7.3 to 3.3)
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...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 32671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 32673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 32673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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.71kH98nwRJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1448, passed=32076
Got 32076 stars (including 30563 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat
util/solve_plate_with_UCAC5 got 32076 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
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...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.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.rs0XvXMTso (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1526, passed=35727
Got 35727 stars (including 34144 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat
util/solve_plate_with_UCAC5 got 35727 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
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...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 35407 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 35406 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 35406 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Saving fully-calibrated image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-18-13_20.00sec_-4.90C_LIGHTs_0148.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-08-Q1b1x1_002416_TTUQ1b1x1_27543_VETCrbNx/wcs_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149.fits
Preparing the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53125.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52967.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out52983.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out51980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52902.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 51711_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 51711_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:17:59.68 -04:19:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51715_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 51715_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 10:49:47.01 -05:17:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 1.151 3776972907000710016 162.44607878193 -05.29158033935 14.3976 13.8956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51717_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 51717_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:39:08.86 -00:03:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.825 3795768027485258368 174.78613295166 -00.05617678187 14.7170 14.2434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51722_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 51722_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:35:30.10 +02:10:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51723_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 51723_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:25:45.02 +01:31:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51725_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 51725_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:32:30.09 +00:00:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51727_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 51727_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:24:33.63 -04:09:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.356 3787056180246613120 171.14003546040 -04.16329074296 13.1031 12.6388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51728_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 51728_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:34:19.07 -03:15:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51980_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
Preparing report for the candidate 51980_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
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Considering the candidate 52143_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
Preparing report for the candidate 52143_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
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Considering the candidate 52212_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
Preparing report for the candidate 52212_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
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Considering the candidate 52251_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52251_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:39:32.81 +01:49:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52298_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
Preparing report for the candidate 52298_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
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Considering the candidate 52360_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52360_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:37:10.27 -00:48:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52452_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52452_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:02:26.07 +00:05:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52570_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52570_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:39:39.90 +02:11:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52620_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
Preparing report for the candidate 52620_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
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Considering the candidate 52654_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52654_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:38:21.53 +02:13:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52665_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
Preparing report for the candidate 52665_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
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Considering the candidate 52704_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52704_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:04:37.83 -07:02:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52722_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52722_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:28:57.67 -06:48:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52744_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52744_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:31:18.98 -06:36:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52777_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52777_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:02:01.76 -06:57:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52811_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52811_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:39:49.02 +02:21:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52814_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52814_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 10:59:42.87 +02:30:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52820_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52820_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 10:55:07.32 -03:56:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.884 3801186936183014784 163.78094879337 -03.94874337195 15.3526 14.9284 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52825_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52825_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:39:28.09 +01:49:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52875_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52875_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:35:18.50 -04:25:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52902_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
Preparing report for the candidate 52902_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
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Considering the candidate 52903_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52903_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:31:55.32 -00:32:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.75, MAG_FAINT_SEARCH_LIMIT=15.73)GAIADR2_OUTPUT=# 1.793 3797203439915306752 172.98030300588 -00.53879063753 14.6614 13.9970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52904_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52904_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:04:50.38 -06:38:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.352 3787582300856185600 166.20980129088 -06.63760777500 14.1451 13.0341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52914_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52914_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:09:13.44 -04:48:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 2.043 3788230772198011520 167.30654791596 -04.81670998171 14.7900 14.2991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52924_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52924_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:33:47.52 -07:01:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 0.592 3592987262638157184 173.44783469754 -07.01999023286 14.7850 14.3061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52936_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52936_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:33:46.51 -02:26:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52946_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52946_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 10:41:04.97 +01:36:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52950_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52950_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:15:12.69 -06:10:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52956_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52956_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:28:45.07 -04:28:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52957_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52957_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:27:05.07 -05:21:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52965_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52965_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 10:38:47.57 -04:23:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.952 3777669069659476992 159.69867882231 -04.39399387740 14.8211 14.3383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52967_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52967_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:20:38.16 -04:44:54.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)
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Considering the candidate 52974_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52974_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:36:55.56 -06:46:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.505 3593335567306082432 174.23166215021 -06.77477471863 14.6374 14.0685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52982_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52982_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:16:53.85 +02:55:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 1.859 3811779699924586880 169.22454256672 +02.92851153355 14.7656 14.0651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52983_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52983_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 10:58:12.75 +01:36:22.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)
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Considering the candidate 52987_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52987_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:39:36.05 -01:57:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 0.132 3793007188148030336 174.90021214201 -01.95981412597 14.9757 14.2466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52989_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 52989_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 10:55:40.40 -06:21:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.780 3764591443999250688 163.91879934432 -06.35786725412 14.8314 14.3136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53001_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53001_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:22:09.45 -06:12:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 1.319 3785628159455391872 170.53971105405 -06.21431688403 14.9520 14.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53005_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53005_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:31:42.89 +01:39:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 0.553 3799943972647623808 172.92856592768 +01.66183555845 14.8096 14.1899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53008_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53008_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:24:48.69 -06:42:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 0.680 3785352525634274176 171.20298842335 -06.71020720547 14.8710 14.3928 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 53043_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53043_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:20:23.72 +02:20:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.129 3810936065268466304 170.09883539873 +02.34551960060 14.6186 14.0664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53045_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53045_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:18:46.62 -06:17:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53051_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53051_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:09:52.53 -04:28:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 1.506 3788526609545255424 167.46897246946 -04.46975969072 15.1890 14.6358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53062_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53062_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:32:11.37 -05:32:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53063_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53063_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:35:19.64 +00:00:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 1.084 3797296142489584512 173.83205743475 +00.01246536055 14.7726 14.2275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53086_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53086_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:07:49.14 +02:21:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53099_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53099_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:28:46.04 -03:22:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 3.328 3787217125556183296 172.19246051944 -03.37465234183 14.8395 14.3432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53107_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53107_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:36:47.64 -01:52:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 0.525 3793799420635384576 174.19861286385 -01.87523143716 14.8317 14.3035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53108_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53108_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:34:02.48 -06:19:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 2.762 3593610479572825856 173.51102314616 -06.32212207279 14.9219 14.9677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53110_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53110_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:32:43.57 -06:12:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.786 3593290418609889792 173.18147942228 -06.21045951695 14.7603 14.2478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53111_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53111_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:35:34.71 -01:11:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53120_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53120_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:30:32.72 +01:08:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.957 3798406786672784768 172.63632894448 +01.13487313056 14.7089 14.1673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53125_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53125_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:17:03.46 +01:58:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.053 3810907581045287424 169.26464132737 +01.96895149314 14.6765 14.1786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53134_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53134_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:27:48.13 +02:32:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 1.419 3800294132741292800 171.95028908422 +02.54933610752 14.6732 13.8626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53172_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 53172_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks
**** FOUND 11:36:00.32 -00:29:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.299 3794240634035740032 174.00135608501 -00.49466311963 14.6685 14.0309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 14520_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149
The candidate 14520_fd_Leo-08-Q1b1x1_2026-04-16_00-23-12_20.00sec_-5.00C_LIGHTs_0149 did not pass the final checks