This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.2066* 10 13 23.10 +15 31 58.0 10.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7066,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2066 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.2066* 09 49 27.20 +16 15 38.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7066,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2066 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 06.2066* 09 38 21.97 +17 06 26.7 13.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7066,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2066 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.2066* 09 26 03.95 +13 37 11.9 14.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7066,14.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2066 14.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.2066* 09 48 27.41 +11 38 47.3 15.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J147.1142+11.6463,2461136.7066,14.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J147.1142+11.6463 20260406.2066 14.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.2066* 09 39 14.46 +09 53 25.0 14.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7066,14.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2066 14.88CV 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: 2461058.86919819 18.01.2026 08:51:28.724 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
First image: 2461058.86919819 18.01.2026 08:51:28.724 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Last image: 2461136.70694273 06.04.2026 04:57:49.852 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.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.: -7.51
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: 4 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): 6468
Objects passed selection criteria: 6464
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 6215
Average stars matched: 6071.75 (97.6951 %)
Memory usage VmPeak: 112604 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:02:31 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: 2461058.86919819 18.01.2026 08:51:28.724 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
First image: 2461058.86919819 18.01.2026 08:51:28.724 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Last image: 2461136.70694273 06.04.2026 04:57:49.852 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 66
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.22
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: 22 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): 36981
Objects passed selection criteria: 36882
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: 35392.8
Average stars matched: 34236.8 (96.7338 %)
Memory usage VmPeak: 139216 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:03:50 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.70626896
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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
Saving wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits to local_wcs_cache/
'wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits'
wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits exists and is non-empty
Saving wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits to local_wcs_cache/
'wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits' -> 'local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits'
wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits exists and is non-empty
Saving wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits'
wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits exists and is non-empty
Saving wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:46:34.262 +13:59:45.34
Second-epoch image center 09:46:54.460 +14:00:12.79
Angular distance between the image centers 0.0820 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:34.262 +13:59:45.34
Second-epoch image center 09:46:54.136 +14:00:39.12
Angular distance between the image centers 0.0817 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 09:46:54.460 +14:00:12.79
Second-epoch second image center 09:46:54.136 +14:00:39.12
Angular distance between the image centers 0.00743 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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.qBeeXhRwLu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits &> /tmp/tmp.KYAtvR3okP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits &> /tmp/tmp.wPArV9xsE9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits &> /tmp/tmp.T56CIjDZu3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
The reference image (wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits) and catalog (wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat) found
'wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat' -> 'wcsmag.cat'
Read 7958 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.3852 to 154.9366 deg, Dec +8.6225 to +19.2659 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 138.3852 to 154.9366 deg, Dec 8.6225 to 19.2659 deg
Loaded 4773 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): 3901 out of 4125 total matches.
Matched with Tycho-2 4125 out of 7958 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.887154
a=0.000000 b=1.000000 c=22.887154
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
2.1 pix Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
2.6 pix fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
2.6 pix fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
Limiting magnitude estimates:
15.4 mag. Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
15.4 mag. Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
15.2 mag. fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
15.2 mag. fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (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.qBeeXhRwLu (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=534, passed=7958
Got 7958 stars (including 7414 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 7958 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 7691 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 7690 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
WARNING: Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 7690 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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.KYAtvR3okP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=535, passed=8039
Got 8039 stars (including 7496 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat
util/solve_plate_with_UCAC5 got 8039 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 7747 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 7747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
WARNING: Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 7747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 913 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits -region wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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.wPArV9xsE9 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=426, passed=7566
Got 7566 stars (including 7133 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat
util/solve_plate_with_UCAC5 got 7566 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 7414 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 7411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
WARNING: Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 7411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits -region wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.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.T56CIjDZu3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=420, passed=7510
Got 7510 stars (including 7086 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat
util/solve_plate_with_UCAC5 got 7510 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 7374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 7373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
WARNING: Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 7373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 913 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits -region wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits'
Saving fully-calibrated image wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits'
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits'
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits'
Preparing the HTML report for the field Leo-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20391.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20377_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 20377_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 10:15:06.91 +12:29:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.613 3880874625521522048 153.77862657411 +12.50039035794 12.3683 11.8567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20391_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
Preparing report for the candidate 20391_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20421_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 20421_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:57:57.95 +15:51:32.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Leo-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:13:23.10 +15:31:58.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits exists and is non-empty
wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits exists and is non-empty
wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:46:34.262 +13:59:45.34
Second-epoch image center 09:46:54.460 +14:00:12.79
Angular distance between the image centers 0.0820 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:34.262 +13:59:45.34
Second-epoch image center 09:46:54.136 +14:00:39.12
Angular distance between the image centers 0.0817 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 09:46:54.460 +14:00:12.79
Second-epoch second image center 09:46:54.136 +14:00:39.12
Angular distance between the image centers 0.00743 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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.DJvLLYIdMb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits &> /tmp/tmp.iX0skPoZCZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits &> /tmp/tmp.kWZDXFPdM4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits &> /tmp/tmp.HsgCLsXoqu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
The reference image (wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits) and catalog (wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat) found
'wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat' -> 'wcsmag.cat'
Read 43775 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.3793 to 154.9626 deg, Dec +8.6120 to +19.2857 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 138.3793 to 154.9626 deg, Dec 8.6120 to 19.2857 deg
Loaded 4796 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): 3707 out of 4153 total matches.
Matched with Tycho-2 4153 out of 43775 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.771580
a=0.000000 b=1.000000 c=22.771580
From vast_summary.log: estimated ref. image limiting mag.: -7.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.55
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.55
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 41 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
2.0 pix Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
2.2 pix fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
2.2 pix fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
Limiting magnitude estimates:
15.6 mag. Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
15.5 mag. Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
15.4 mag. fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
15.4 mag. fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (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.DJvLLYIdMb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1969, passed=43757
Got 43757 stars (including 41703 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 43757 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 42352 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 42347 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
WARNING: Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 42347 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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.iX0skPoZCZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1988, passed=43712
Got 43712 stars (including 41658 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat
util/solve_plate_with_UCAC5 got 43712 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 42220 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 42218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
WARNING: Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 42219 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 908 stars left (next iteration limit 998)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits -region wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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.kWZDXFPdM4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1713, passed=39495
Got 39495 stars (including 37730 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat
util/solve_plate_with_UCAC5 got 39495 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 38797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 38799 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
WARNING: Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 38800 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 909 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits -region wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.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.HsgCLsXoqu (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1785, passed=39501
Got 39501 stars (including 37667 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat
util/solve_plate_with_UCAC5 got 39501 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 38858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 38858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
WARNING: Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 38857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 909 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits -region wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.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-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/wcs_Leo-04-Q2b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Saving fully-calibrated image wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/wcs_Leo-04-Q2b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-56-51_20.00sec_-5.00C_LIGHT_0156.fits
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Leo-04-Q2b1x1_000009_TTUQ2b1x1_5367_gemRB2YD/wcs_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157.fits
Preparing the HTML report for the field Leo-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52865.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53024.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 52485_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52485_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 10:06:04.39 +12:35:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.723 3881618651296566400 151.51781243957 +12.58942620431 14.7287 14.1992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52488_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52488_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:28:36.10 +14:34:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 1.002 618355929188299648 142.15067102391 +14.57798145193 14.3476 13.8575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52490_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52490_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:39:26.34 +14:13:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 0.750 617688285112042240 144.85994735336 +14.22116762209 14.3632 13.5959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52496_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52496_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:41:47.91 +11:28:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.530 613663797676628992 145.44984190475 +11.48157634605 14.3021 13.7981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52501_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52501_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 10:05:32.54 +13:30:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.235 3881937574092313984 151.38494498619 +13.51560333954 13.1628 12.7365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52502_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52502_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:24:41.37 +11:37:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52516_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52516_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 10:13:23.10 +15:31:58.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52550_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
Preparing report for the candidate 52550_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
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Considering the candidate 52561_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52561_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:30:25.86 +12:57:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52565_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52565_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:51:35.86 +17:28:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52582_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52582_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:39:00.82 +14:25:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52613_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
Preparing report for the candidate 52613_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
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Considering the candidate 52654_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52654_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:31:05.19 +11:30:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52687_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52687_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:39:26.92 +16:46:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52714_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52714_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:31:51.19 +17:15:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52715_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52715_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:29:04.57 +17:51:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52728_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52728_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:44:02.21 +17:34:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52737_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52737_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:52:12.27 +16:27:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52743_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52743_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 10:08:38.45 +11:59:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52753_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52753_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:30:38.58 +17:04:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.342 631317792595150720 142.66065068095 +17.07286623806 14.1208 13.4621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52811_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52811_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:54:27.13 +09:50:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.033 3878982537808764544 148.61316876007 +09.84813075840 14.5391 13.9604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52829_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52829_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:31:59.83 +09:40:56.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52833_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52833_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:30:19.50 +15:12:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 2.597 618593625562948224 142.58187550309 +15.20752184423 14.3995 13.2106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52860_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52860_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:39:22.97 +13:17:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52865_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52865_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:32:17.10 +09:40:56.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)
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Considering the candidate 52869_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52869_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:29:08.84 +10:26:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 0.878 589382938803326976 142.28662139087 +10.43429344626 14.7712 14.3089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52878_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52878_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:29:23.54 +15:42:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 0.918 619054393950285824 142.34784679209 +15.71372608064 14.8558 14.3874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52880_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52880_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:34:34.23 +16:56:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.314 620743656127286528 143.64265405408 +16.94375064352 14.2910 13.3250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52888_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52888_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:40:35.40 +15:02:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 1.568 618021712013237760 145.14746682765 +15.04712121681 14.9137 14.3878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52896_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
Preparing report for the candidate 52896_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
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Considering the candidate 52897_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52897_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:23:55.58 +12:47:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52901_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52901_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:39:16.99 +13:43:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 2.279 617587679798137344 144.82023174113 +13.72448149787 14.9052 14.2963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52909_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52909_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:34:05.14 +10:06:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 1.832 589439357493427328 143.52184320295 +10.10862924357 15.1693 14.5598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52918_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52918_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:27:26.30 +11:42:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 0.393 592911615214100352 141.85969283706 +11.71559117094 14.9970 14.5014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52922_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52922_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:41:09.25 +13:54:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52924_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52924_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:46:04.68 +16:29:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52938_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52938_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:47:33.88 +14:09:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52971_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52971_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks
**** FOUND 09:31:17.23 +12:14:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 0.680 593036959539538176 142.82171348059 +12.23966046151 14.8605 14.4093 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 52981_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157
The candidate 52981_fd_Leo-04-Q2b1x1_2026-04-05_23-57-49_20.00sec_-5.00C_LIGHT_0157 did not pass the final checks