This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 10 09.4526 2461322.9526 13.49 10:29:34.50 +14:06:42.9
227.20783 54.50470 galactic Leo Second-epoch detections are separated by 1.3" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.94 Aurora -0 -0 1 13.7 0 -0
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:29:34.50 +14:06:42.9: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:29:34.50 +14:06:42.9: 15.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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 10 09.4526* 10 29 34.50 +14 06 42.9 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461322.9526,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4526 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.4526 2461322.9526 13.24 10:45:47.59 +14:21:19.7
230.13743 58.09205 galactic Leo Second-epoch detections are separated by 0.7" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.42 Isis -1 0 1 13.6 0 -0
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:45:47.59 +14:21:19.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:45:47.59 +14:21:19.7: 15.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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 10 09.4526* 10 45 47.59 +14 21 19.7 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461322.9526,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4526 13.24CV 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
Mean magnitude and position on the discovery images:
2026 10 09.4526 2461322.9526 13.59 10:57:37.85 +13:52:26.3
233.74390 60.34311 galactic Leo Second-epoch detections are separated by 1.9" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.187 Lamberta 1 1 1 13.6 0 -0
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:57:37.85 +13:52:26.3: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:57:37.85 +13:52:26.3: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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 10 09.4526* 10 57 37.85 +13 52 26.3 13.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461322.9526,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.4526 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461171.68283635 11.05.2026 04:23:07.061 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
First image: 2461171.68283635 11.05.2026 04:23:07.061 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Last image: 2461322.95284972 09.10.2026 10:51:56.216 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 4863
Objects passed selection criteria: 4838
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 3396.25
Average stars matched: 3124.25 (91.9912 %)
Memory usage VmPeak: 231204 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Oct 9 06:14:24 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: 2461171.68283635 11.05.2026 04:23:07.061 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
First image: 2461171.68283635 11.05.2026 04:23:07.061 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Last image: 2461322.95284972 09.10.2026 10:51:56.216 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 129
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.03
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 13 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 26383
Objects passed selection criteria: 26294
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 19455
Average stars matched: 17732.5 (91.1462 %)
Memory usage VmPeak: 248560 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Oct 9 06:15:09 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
SExtractor catalog cache: saved Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.cat to cache
SExtractor catalog cache: saved Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.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-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461322.95238311
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-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits exists and is non-empty
wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits exists and is non-empty
wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits exists and is non-empty
wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits (1st reference image)
verification OK: wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:40:00.118 +14:00:12.76 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits (1st new image)
verification OK: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
Image size: 941.4'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:39:57.403 +13:57:47.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:40:00.118 +14:00:12.76
Second-epoch image center 10:39:57.403 +13:57:47.21
Angular distance between the image centers 0.0419 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits (2nd new image)
verification OK: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Image size: 941.3'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:39:56.612 +13:57:33.75 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:40:00.118 +14:00:12.76
Second-epoch image center 10:39:56.612 +13:57:33.75
Angular distance between the image centers 0.0464 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:39:57.403 +13:57:47.21
Second-epoch second image center 10:39:56.612 +13:57:33.75
Angular distance between the image centers 0.00492 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits &> /tmp/tmp.Twq4MFrgzB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits &> /tmp/tmp.fsO4ETiNAg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits &> /tmp/tmp.bVDhKu5IiU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits &> /tmp/tmp.MlK7YQL4vR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.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-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
Found non-empty wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
The reference image (wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits) and catalog (wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat) found
'wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat' -> 'wcsmag.cat'
Read 5744 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7220 to 168.1826 deg, Dec +8.6400 to +19.2604 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 151.7220 to 168.1826 deg, Dec 8.6400 to 19.2604 deg
Loaded 4240 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): 3428 out of 3506 total matches.
Matched with Tycho-2 3506 out of 5744 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.709950
a=0.000000 b=1.000000 c=22.709950
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5744 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7220 to 168.1826 deg, Dec +8.6400 to +19.2604 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 151.7220 to 168.1826 deg, Dec 8.6400 to 19.2604 deg
Loaded 4240 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): 3428 out of 3506 total matches.
Matched with Tycho-2 3506 out of 5744 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Forced-photometry filter: calibrated wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits -> calib.txt_param_ref_wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits (aperture=6.3)
Read 5709 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7036 to 168.1827 deg, Dec +8.6403 to +19.2435 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 151.7036 to 168.1827 deg, Dec 8.6403 to 19.2435 deg
Loaded 4243 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): 3432 out of 3504 total matches.
Matched with Tycho-2 3504 out of 5709 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Forced-photometry filter: calibrated wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits -> calib.txt_param_ref_wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
2.4 pix Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
2.3 pix fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
2.3 pix fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Limiting magnitude estimates:
15.4 mag. Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
15.4 mag. Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
14.4 mag. fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
14.4 mag. fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.4 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.Twq4MFrgzB (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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.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-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits' -> 'wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat corresponding to the image wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat corresponding to the image wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=319, bad_region=1440, passed=5744
Got 5744 stars (including 4050 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
util/solve_plate_with_UCAC5 got 5744 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 3634 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3630 matched stars entering correct_measured_positions(), 3630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3630 matched stars entering correct_measured_positions(), 4590 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 3633 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3629 matched stars entering correct_measured_positions(), 4590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 3629 matched stars entering correct_measured_positions(), 4590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 3629 stars left (next iteration limit 3993)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits N_match=3629 sigma_overall_arcsec=0.365 sigma_q1_arcsec=0.336 sigma_q2_arcsec=0.368 sigma_q3_arcsec=0.373 sigma_q4_arcsec=0.393 n_q1=1157 n_q2=636 n_q3=1245 n_q4=591 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits -region wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.fsO4ETiNAg (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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.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-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits' -> 'wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=309, bad_region=1424, passed=5709
Got 5709 stars (including 4039 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat
util/solve_plate_with_UCAC5 got 5709 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.2)
Done reading UCAC5 zone files...
Matched 3628 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3625 matched stars entering correct_measured_positions(), 3625 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3625 matched stars entering correct_measured_positions(), 4562 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.2)
Done reading UCAC5 zone files...
Matched 3628 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3622 matched stars entering correct_measured_positions(), 4562 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 3622 matched stars entering correct_measured_positions(), 4562 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 3622 stars left (next iteration limit 3987)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits N_match=3622 sigma_overall_arcsec=0.354 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.366 sigma_q3_arcsec=0.364 sigma_q4_arcsec=0.364 n_q1=1144 n_q2=651 n_q3=1241 n_q4=586 worst_quadrant_to_overall_ratio=1.032
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits -region wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.bVDhKu5IiU (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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
Checking if the catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
WCS catalog name: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=222, bad_region=574, passed=3108
Got 3108 stars (including 2338 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat
util/solve_plate_with_UCAC5 got 3108 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.2)
Done reading UCAC5 zone files...
Matched 1998 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1991 matched stars entering correct_measured_positions(), 1991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1991 matched stars entering correct_measured_positions(), 2646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.2)
Done reading UCAC5 zone files...
Matched 1996 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1991 matched stars entering correct_measured_positions(), 2646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 1991 matched stars entering correct_measured_positions(), 2646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 1991 stars left (next iteration limit 2190)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1991 robust_rms=6.820 arcsec worst_region_rms=10.932 arcsec outer_annulus_rms=10.932 arcsec
SIP_REFIT: SIP order 3 trial: matched=1991 robust_rms=0.522 arcsec worst_region_rms=0.567 arcsec outer_annulus_rms=0.567 arcsec
SIP_REFIT: SIP order 5 trial: matched=1991 robust_rms=0.401 arcsec worst_region_rms=0.483 arcsec outer_annulus_rms=0.483 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1991 robust_rms_before=1.895 arcsec robust_rms_before_corrected=0.406 arcsec robust_rms_after=0.401 arcsec worst_region_rms_before=0.517 worst_region_rms_after=0.483 outer_annulus_rms_before=1.742 outer_annulus_rms_after=0.483
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.517 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits worst_region_rms_kept=0.517 arcsec robust_rms_kept=0.406 arcsec matched=1991
WCS_QUALITY_DIAG: file=fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits N_match=1991 sigma_overall_arcsec=0.420 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.452 sigma_q3_arcsec=0.418 sigma_q4_arcsec=0.414 n_q1=642 n_q2=342 n_q3=645 n_q4=362 worst_quadrant_to_overall_ratio=1.078
The image catalog is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits -region wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.MlK7YQL4vR (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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Checking if the catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
WCS catalog name: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=266, bad_region=599, passed=3167
Got 3167 stars (including 2340 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat
util/solve_plate_with_UCAC5 got 3167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.2)
Done reading UCAC5 zone files...
Matched 1996 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1989 matched stars entering correct_measured_positions(), 1989 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1989 matched stars entering correct_measured_positions(), 2675 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.2)
Done reading UCAC5 zone files...
Matched 1995 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1990 matched stars entering correct_measured_positions(), 2675 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 1990 matched stars entering correct_measured_positions(), 2675 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 1990 stars left (next iteration limit 2187)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1990 robust_rms=6.891 arcsec worst_region_rms=10.407 arcsec outer_annulus_rms=10.407 arcsec
SIP_REFIT: SIP order 3 trial: matched=1990 robust_rms=0.539 arcsec worst_region_rms=0.633 arcsec outer_annulus_rms=0.532 arcsec
SIP_REFIT: SIP order 5 trial: matched=1990 robust_rms=0.388 arcsec worst_region_rms=0.475 arcsec outer_annulus_rms=0.475 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1990 robust_rms_before=1.911 arcsec robust_rms_before_corrected=0.407 arcsec robust_rms_after=0.388 arcsec worst_region_rms_before=0.511 worst_region_rms_after=0.475 outer_annulus_rms_before=1.735 outer_annulus_rms_after=0.475
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.511 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits worst_region_rms_kept=0.511 arcsec robust_rms_kept=0.407 arcsec matched=1990
WCS_QUALITY_DIAG: file=fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits N_match=1990 sigma_overall_arcsec=0.431 sigma_q1_arcsec=0.419 sigma_q2_arcsec=0.512 sigma_q3_arcsec=0.418 sigma_q4_arcsec=0.425 n_q1=634 n_q2=337 n_q3=662 n_q4=357 worst_quadrant_to_overall_ratio=1.188
The image catalog is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits -region wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits to local_wcs_cache/
'wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits' -> 'local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits'
Saving the final (post-refit) wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits to local_wcs_cache/
'wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits' -> 'local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits'
Saving the final (post-refit) wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits to local_wcs_cache/
'wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits' -> 'local_wcs_cache/wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits'
Saving the final (post-refit) wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits to local_wcs_cache/
'wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits' -> 'local_wcs_cache/wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits sigma_overall=0.365 worst_q_ratio=1.077
ref2=Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits sigma_overall=0.354 worst_q_ratio=1.032
new1=fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits sigma_overall=0.420 worst_q_ratio=1.078
new2=fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits sigma_overall=0.431 worst_q_ratio=1.188
reference average sigma_overall=0.3595 worst_q_ratio=1.0545
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141_astrometric_residuals.png (3629 matched stars from wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142_astrometric_residuals.png (3622 matched stars from wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596_astrometric_residuals.png (1991 matched stars from wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597_astrometric_residuals.png (1990 matched stars from wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits'
Saving fully-calibrated image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits'
Preparing the HTML report for the field Leo-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Leo-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
SExtractor catalog cache: saved Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.cat to cache
SExtractor catalog cache: saved Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.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-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Creating symlink local_wcs_cache/wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Checking 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-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits exists and is non-empty
wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits exists and is non-empty
wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits exists and is non-empty
wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits (1st reference image)
verification OK: wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:40:00.118 +14:00:12.76 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits (1st new image)
verification OK: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
Image size: 941.4'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:39:57.403 +13:57:47.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:40:00.118 +14:00:12.76
Second-epoch image center 10:39:57.403 +13:57:47.21
Angular distance between the image centers 0.0419 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits (2nd new image)
verification OK: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Image size: 941.3'x624.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:39:56.612 +13:57:33.75 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:40:00.118 +14:00:12.76
Second-epoch image center 10:39:56.612 +13:57:33.75
Angular distance between the image centers 0.0464 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:39:57.403 +13:57:47.21
Second-epoch second image center 10:39:56.612 +13:57:33.75
Angular distance between the image centers 0.00492 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits &> /tmp/tmp.BzATDmW05q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits &> /tmp/tmp.2ubbmgarIS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits &> /tmp/tmp.0rxTJUgyuI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits &> /tmp/tmp.Y64MG5iepg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.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-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
Found non-empty wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
The reference image (wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits) and catalog (wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat) found
'wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat' -> 'wcsmag.cat'
Read 29548 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7119 to 168.2363 deg, Dec +8.6400 to +19.2694 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 151.7119 to 168.2363 deg, Dec 8.6400 to 19.2694 deg
Loaded 4250 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): 3390 out of 3597 total matches.
Matched with Tycho-2 3597 out of 29548 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.581200
a=0.000000 b=1.000000 c=22.581200
From vast_summary.log: estimated ref. image limiting mag.: -7.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.55
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.55
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29548 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7119 to 168.2363 deg, Dec +8.6400 to +19.2694 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 151.7119 to 168.2363 deg, Dec 8.6400 to 19.2694 deg
Loaded 4250 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): 3390 out of 3597 total matches.
Matched with Tycho-2 3597 out of 29548 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Forced-photometry filter: calibrated wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits -> calib.txt_param_ref_wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits (aperture=4.9)
Read 29453 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7036 to 168.1940 deg, Dec +8.6403 to +19.2611 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 151.7036 to 168.1940 deg, Dec 8.6403 to 19.2611 deg
Loaded 4245 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): 3386 out of 3596 total matches.
Matched with Tycho-2 3596 out of 29453 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Forced-photometry filter: calibrated wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits -> calib.txt_param_ref_wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 85 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
2.2 pix Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
2.3 pix fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
2.3 pix fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Limiting magnitude estimates:
15.6 mag. Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
15.5 mag. Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
14.6 mag. fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
14.6 mag. fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 13.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BzATDmW05q (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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.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-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits' -> 'wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat corresponding to the image wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat corresponding to the image wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1176, bad_region=5538, passed=29533
Got 29533 stars (including 23167 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
util/solve_plate_with_UCAC5 got 29533 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4505 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4499 matched stars entering correct_measured_positions(), 4499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4499 matched stars entering correct_measured_positions(), 25250 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4506 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4496 matched stars entering correct_measured_positions(), 25250 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4496 matched stars entering correct_measured_positions(), 25241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4496 stars left (next iteration limit 4948)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits N_match=4496 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.336 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.380 n_q1=1458 n_q2=789 n_q3=1504 n_q4=745 worst_quadrant_to_overall_ratio=1.053
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits -region wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.2ubbmgarIS (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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.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-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits' -> 'wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS-calibrated image found: wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Checking if the catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS catalog name: wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1170, bad_region=5455, passed=29442
Got 29442 stars (including 23120 good ones) from the SExtractor catalog wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat
util/solve_plate_with_UCAC5 got 29442 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4505 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 4495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 25215 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4505 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4493 matched stars entering correct_measured_positions(), 25215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4493 matched stars entering correct_measured_positions(), 25215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4493 stars left (next iteration limit 4944)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits N_match=4493 sigma_overall_arcsec=0.356 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.366 sigma_q3_arcsec=0.360 sigma_q4_arcsec=0.367 n_q1=1453 n_q2=776 n_q3=1521 n_q4=743 worst_quadrant_to_overall_ratio=1.030
The image catalog is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits -region wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.0rxTJUgyuI (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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
Checking if the catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
WCS catalog name: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=636, bad_region=2300, passed=17531
Got 17531 stars (including 14663 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat
util/solve_plate_with_UCAC5 got 17531 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4233 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4220 matched stars entering correct_measured_positions(), 4220 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4220 matched stars entering correct_measured_positions(), 15786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4232 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4220 matched stars entering correct_measured_positions(), 15786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4220 matched stars entering correct_measured_positions(), 15786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4220 stars left (next iteration limit 4642)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4220 robust_rms=6.618 arcsec worst_region_rms=11.185 arcsec outer_annulus_rms=11.185 arcsec
SIP_REFIT: SIP order 3 trial: matched=4220 robust_rms=0.561 arcsec worst_region_rms=0.614 arcsec outer_annulus_rms=0.614 arcsec
SIP_REFIT: SIP order 5 trial: matched=4220 robust_rms=0.449 arcsec worst_region_rms=0.509 arcsec outer_annulus_rms=0.509 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4220 robust_rms_before=1.915 arcsec robust_rms_before_corrected=0.430 arcsec robust_rms_after=0.449 arcsec worst_region_rms_before=0.523 worst_region_rms_after=0.509 outer_annulus_rms_before=1.797 outer_annulus_rms_after=0.509
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.523 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits worst_region_rms_kept=0.523 arcsec robust_rms_kept=0.430 arcsec matched=4220
WCS_QUALITY_DIAG: file=fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits N_match=4220 sigma_overall_arcsec=0.434 sigma_q1_arcsec=0.433 sigma_q2_arcsec=0.471 sigma_q3_arcsec=0.434 sigma_q4_arcsec=0.413 n_q1=1404 n_q2=676 n_q3=1366 n_q4=774 worst_quadrant_to_overall_ratio=1.086
The image catalog is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits -region wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Y64MG5iepg (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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Checking if the catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
WCS catalog name: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=642, bad_region=2339, passed=17626
Got 17626 stars (including 14767 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat
util/solve_plate_with_UCAC5 got 17626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.2)
Done reading UCAC5 zone files...
Matched 4227 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4217 matched stars entering correct_measured_positions(), 4217 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4217 matched stars entering correct_measured_positions(), 15846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.2)
Done reading UCAC5 zone files...
Matched 4228 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4218 matched stars entering correct_measured_positions(), 15846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4218 matched stars entering correct_measured_positions(), 15846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4218 stars left (next iteration limit 4638)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4218 robust_rms=6.687 arcsec worst_region_rms=10.905 arcsec outer_annulus_rms=10.905 arcsec
SIP_REFIT: SIP order 3 trial: matched=4218 robust_rms=0.574 arcsec worst_region_rms=0.672 arcsec outer_annulus_rms=0.605 arcsec
SIP_REFIT: SIP order 5 trial: matched=4218 robust_rms=0.439 arcsec worst_region_rms=0.527 arcsec outer_annulus_rms=0.527 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4218 robust_rms_before=1.928 arcsec robust_rms_before_corrected=0.426 arcsec robust_rms_after=0.439 arcsec worst_region_rms_before=0.529 worst_region_rms_after=0.527 outer_annulus_rms_before=1.764 outer_annulus_rms_after=0.527
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.529 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits worst_region_rms_kept=0.529 arcsec robust_rms_kept=0.426 arcsec matched=4218
WCS_QUALITY_DIAG: file=fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits N_match=4218 sigma_overall_arcsec=0.431 sigma_q1_arcsec=0.452 sigma_q2_arcsec=0.453 sigma_q3_arcsec=0.408 sigma_q4_arcsec=0.420 n_q1=1408 n_q2=674 n_q3=1374 n_q4=762 worst_quadrant_to_overall_ratio=1.051
The image catalog is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits -region wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-15_20.00sec_-0.00C_LIGHT_0596.fits
Saving fully-calibrated image wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.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_2026-10-09_CI_Leo-05-Q2b1x1_061201_TTUQ2b1x1_3755148_CMF3rYUa/wcs_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597.fits
Preparing the HTML report for the field Leo-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:31:01.69 +17:50:08.5: 12.20 +/- 0.01 detection
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:31:01.69 +17:50:08.5: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry filter REJECTED candidate at 10:31:01.69 +17:50:08.5: ref_mag=12.21 +/- 0.01 new_mean_mag=12.4984 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:29:34.50 +14:06:42.9: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:45:47.59 +14:21:19.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:29:34.50 +14:06:42.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:57:37.85 +13:52:26.3: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:45:47.59 +14:21:19.7: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q2b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:57:37.85 +13:52:26.3: 15.88 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out34641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36015.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 31746_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 31746_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 31748_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 31748_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 31749_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 31749_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
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Considering the candidate 32030_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 32030_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 32076_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 32076_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 32272_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 32272_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 32506_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 32506_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 32697_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 32697_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 32791_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 32791_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 32950_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 32950_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 32999_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 32999_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 33036_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33036_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 33068_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33068_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 33098_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33098_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 33119_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33119_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 33125_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33125_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 33141_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33141_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 33328_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33328_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 33374_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33374_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 33382_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33382_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 33391_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33391_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 33420_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33420_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 33501_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33501_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 33538_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33538_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 33590_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33590_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 33627_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33627_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 33652_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33652_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 33688_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33688_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 33739_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33739_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 33831_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33831_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 33882_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33882_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 33939_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33939_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 33955_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33955_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 33975_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 33975_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 34018_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34018_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 34020_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34020_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 34028_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34028_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 34208_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34208_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 34230_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34230_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 34358_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34358_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 34408_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34408_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 34434_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34434_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 34476_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34476_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 34570_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34570_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 34641_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
Preparing report for the candidate 34641_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
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Considering the candidate 34651_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34651_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 34665_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
Preparing report for the candidate 34665_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
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Considering the candidate 34691_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34691_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 34717_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34717_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 34721_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34721_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 34774_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34774_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 34810_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34810_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 34831_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34831_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 34917_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34917_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 34935_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 34935_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 35122_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35122_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 35214_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35214_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 35256_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35256_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 35361_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35361_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 35678_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35678_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 35745_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35745_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 35828_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35828_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 35851_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35851_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 35874_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35874_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 35884_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35884_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 35931_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35931_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 35963_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35963_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 35999_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 35999_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 36015_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
Preparing report for the candidate 36015_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
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Considering the candidate 36064_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36064_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 36078_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36078_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 36118_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36118_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 36144_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36144_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 36155_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36155_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 36159_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36159_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 36162_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36162_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 36180_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36180_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 36208_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36208_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 36219_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36219_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
**** FOUND 10:48:08.04 +14:13:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36259_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36259_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 36315_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36315_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 36318_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36318_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 36326_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36326_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 36364_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 36364_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 13543_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597
The candidate 13543_fd_Leo-05-Q2b1x1_2026-10-09_05-51-56_20.00sec_0.00C_LIGHT_0597 did not pass the final checks