This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh
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 13.2867* 11 13 40.53 +01 28 31.8 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7867,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2867 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.2867* 11 03 22.06 +02 37 47.3 13.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7867,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2867 13.13CV 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 13.2867* 10 40 44.27 +00 33 51.6 13.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7867,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2867 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.2867* 11 29 05.91 +01 43 53.7 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7867,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2867 14.27CV 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 13.2867* 10 44 24.57 -04 38 35.2 14.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7867,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2867 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461143.78711266 13.04.2026 06:53:16.534 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6346
Objects passed selection criteria: 6336
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 5866.5
Average stars matched: 5714 (97.4005 %)
Memory usage VmPeak: 112184 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 01:55:19 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461143.78711266 13.04.2026 06:53:16.534 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 33273
Objects passed selection criteria: 33223
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 31230
Average stars matched: 30319.2 (97.0837 %)
Memory usage VmPeak: 134724 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 01:56:06 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.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: 2461143.78638204
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
Saving wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits to local_wcs_cache/
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
Saving wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits to local_wcs_cache/
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits'
wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:26.898 -02:00:51.20
Angular distance between the image centers 0.0364 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:29.976 -02:01:13.78
Angular distance between the image centers 0.0298 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:26.898 -02:00:51.20
Second-epoch second image center 11:08:29.976 -02:01:13.78
Angular distance between the image centers 0.01427 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.5Aj6UsrA16
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.uEzFTg0jx6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits &> /tmp/tmp.Dgzabqsj1L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits &> /tmp/tmp.NaRagct7ul
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat' -> 'wcsmag.cat'
Read 6399 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.2436 to 175.0501 deg, Dec -7.2952 to +3.3133 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.2436 to 175.0501 deg, Dec -7.2952 to 3.3133 deg
Loaded 3835 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3238 out of 3372 total matches.
Matched with Tycho-2 3372 out of 6399 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.879752
a=0.000000 b=1.000000 c=22.879752
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.3 pix fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
2.3 pix fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
Limiting magnitude estimates:
15.2 mag. Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.2 mag. Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
14.9 mag. fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
14.9 mag. fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5Aj6UsrA16 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=432, passed=6399
Got 6399 stars (including 5960 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 6399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 6330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 6329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 6329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uEzFTg0jx6 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=407, passed=6519
Got 6519 stars (including 6107 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 6519 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 6416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 6418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 6418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Dgzabqsj1L (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_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.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_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=353, passed=5413
Got 5413 stars (including 5055 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat
util/solve_plate_with_UCAC5 got 5413 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.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.NaRagct7ul (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_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.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_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=355, passed=5314
Got 5314 stars (including 4956 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat
util/solve_plate_with_UCAC5 got 5314 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5283 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5283 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
Saving fully-calibrated image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits'
Preparing the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20537_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 20537_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:00:24.11 -02:42:26.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00920_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 00920_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:11:21.91 -05:53:31.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Creating symlink local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits exists and is non-empty
wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:26.898 -02:00:51.20
Angular distance between the image centers 0.0364 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:29.976 -02:01:13.78
Angular distance between the image centers 0.0298 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:26.898 -02:00:51.20
Second-epoch second image center 11:08:29.976 -02:01:13.78
Angular distance between the image centers 0.01427 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.AZPLtnR6Fq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.IPF9AWWjJX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits &> /tmp/tmp.snuIHG11Hj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits &> /tmp/tmp.l4pUMcws6R
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat' -> 'wcsmag.cat'
Read 34371 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.2400 to 175.0938 deg, Dec -7.3026 to +3.3144 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.2400 to 175.0938 deg, Dec -7.3026 to 3.3144 deg
Loaded 3852 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3086 out of 3398 total matches.
Matched with Tycho-2 3398 out of 34371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774901
a=0.000000 b=1.000000 c=22.774901
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.3 pix fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
2.2 pix fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
Limiting magnitude estimates:
15.3 mag. Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.3 mag. Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
15.0 mag. fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
15.0 mag. fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (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.AZPLtnR6Fq (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1404, passed=34365
Got 34365 stars (including 32904 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 34365 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 33882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 33882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 33882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IPF9AWWjJX (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1420, passed=33111
Got 33111 stars (including 31640 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 33111 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 32671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 32673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 32673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.snuIHG11Hj (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_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.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_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1244, passed=29135
Got 29135 stars (including 27856 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat
util/solve_plate_with_UCAC5 got 29135 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 28931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 28930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 28930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.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.l4pUMcws6R (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_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.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_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1253, passed=29399
Got 29399 stars (including 28090 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat
util/solve_plate_with_UCAC5 got 29399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 29201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 29200 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 29201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Saving fully-calibrated image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.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_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-52-13_20.00sec_-5.00C_LIGHTs_0096.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.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_2026-04-13_CI_Leo-08-Q1b1x1_015414_TTUQ1b1x1_6033_F4QuoVzh/wcs_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097.fits
Preparing the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out51952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52709.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51705_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 51705_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:36:24.06 +00:05:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.67, MAG_FAINT_SEARCH_LIMIT=15.65)GAIADR2_OUTPUT=# 1.939 3797300540536127744 174.09977034213 +00.08383832841 14.1523 13.6846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51708_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 51708_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:17:59.75 -04:19:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51709_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 51709_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:02:52.36 -05:31:37.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51710_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 51710_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:20:23.61 +01:17:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.58, MAG_FAINT_SEARCH_LIMIT=15.56)GAIADR2_OUTPUT=# 3.515 3810609819552494848 170.09758432007 +01.28803781667 15.1389 14.2526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51712_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 51712_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 10:50:56.47 +01:51:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51716_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 51716_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:31:53.26 -02:20:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 0.672 3793579415230441728 172.97174269285 -02.33848506555 13.8592 13.3379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51717_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 51717_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:32:30.27 +00:00:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51718_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 51718_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:04:04.75 +01:12:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51952_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
Preparing report for the candidate 51952_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
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Considering the candidate 52124_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
Preparing report for the candidate 52124_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
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Considering the candidate 52267_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
Preparing report for the candidate 52267_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
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Considering the candidate 52268_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52268_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 10:48:20.57 -00:42:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52282_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52282_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 10:37:41.29 -03:54:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52383_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52383_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 10:39:29.65 +02:20:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52614_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
Preparing report for the candidate 52614_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
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Considering the candidate 52617_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52617_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 10:55:22.96 +03:14:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52662_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52662_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:38:07.68 -05:55:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52709_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
Preparing report for the candidate 52709_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
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Considering the candidate 52715_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52715_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:31:18.92 -06:36:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52725_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52725_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:39:49.13 +02:21:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52762_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52762_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:28:57.75 -06:48:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52844_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52844_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:32:50.68 -02:25:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 1.832 3793388065847688832 173.21107222527 -02.42250012503 14.8129 14.3418 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 52847_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52847_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 10:58:19.07 +02:38:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 2.694 3808786245158024832 164.58013595819 +02.63329198111 15.0531 14.4038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52895_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52895_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:27:31.82 -03:42:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52917_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 52917_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks
**** FOUND 11:26:58.24 -04:33:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 1.316 3786973648154609152 171.74230210051 -04.56651272391 14.9288 14.4399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 04591_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097
The candidate 04591_fd_Leo-08-Q1b1x1_2026-04-13_01-53-16_20.00sec_-4.90C_LIGHTs_0097 did not pass the final checks