This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx
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 06 08.1820 2461199.6820 10.55 10:49:26.54 -05:02:00.5
255.81149 46.37610 galactic Sex Second-epoch detections are separated by 1.9" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3776993655986859648 | 10:49:26.51 -05:02:00.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.476+/-0.034 (K)
Forced photometry on wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits at 10:49:26.54 -05:02:00.5: 11.49 +/- 0.01 detection
Forced photometry on wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits at 10:49:26.54 -05:02:00.5: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
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 06 08.1820* 10 49 26.54 -05 02 00.5 10.6 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3776993655986859648,2461199.6820,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3776993655986859648 20260608.1820 10.55CV 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 06 08.1820 2461199.6820 10.39 10:45:26.75 -04:30:45.3
254.23428 46.10630 galactic Sex Second-epoch detections are separated by 0.7" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3777182948081021696 | 10:45:26.83 -04:30:45.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.307+/-0.032 (F)
Forced photometry on wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits at 10:45:26.75 -04:30:45.3: 11.45 +/- 0.01 detection
Forced photometry on wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits at 10:45:26.75 -04:30:45.3: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.00
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 06 08.1820* 10 45 26.75 -04 30 45.3 10.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3777182948081021696,2461199.6820,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3777182948081021696 20260608.1820 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1820 2461199.6820 10.65 10:48:38.12 -04:52:58.5
255.44853 46.35770 galactic Sex Second-epoch detections are separated by 2.1" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3777046604343677440 | 10:48:38.12 -04:52:57.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.270+/-0.035 (F)
Forced photometry on wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits at 10:48:38.12 -04:52:58.5: 11.94 +/- 0.01 detection
Forced photometry on wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits at 10:48:38.12 -04:52:58.5: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
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 06 08.1820* 10 48 38.12 -04 52 58.5 10.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3777046604343677440,2461199.6820,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3777046604343677440 20260608.1820 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 3
Ref. image: 2461146.71357755 16.04.2026 05:07:23.100 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
First image: 2461146.71357755 16.04.2026 05:07:23.100 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
Last image: 2461199.68229163 08.06.2026 04:22:19.997 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5442
Objects passed selection criteria: 5412
Measurements per detected object (mean, median, min, max): 2.0 2.0 2 3
Measurements per selected object (mean, median, min, max): 2.0 2.0 2 3
Average stars detected per image: 3948.33
Average stars matched: 3894 (98.6239 %)
Memory usage VmPeak: 111716 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 00:37:36 CDT 2026
Host name: tau
***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.71357755 16.04.2026 05:07:23.100 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
First image: 2461146.71357755 16.04.2026 05:07:23.100 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
Last image: 2461199.68229163 08.06.2026 04:22:19.997 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 11 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 29240
Objects passed selection criteria: 29113
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 16865.8
Average stars matched: 16389.5 (97.1762 %)
Memory usage VmPeak: 133760 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 8 00:38:00 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
Last image: 2461199.68165244 08.06.2026 04:21:24.771 UTC
ERROR running VaST on the field Leo-08-Q1b1x1 (less than 4 images processed)
exp_start= 16.04.2026 05:07:23.100 exp= 20.000 JD= 2461146.71357755 ap= 6.5 rotation= 0.000 *detected= 6049 *matched= 6049 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
exp_start= 11.05.2026 04:15:03.100 exp= 20.000 JD= 2461171.67723495 ap= 6.5 rotation= -0.773 *detected= 5598 *matched= 5441 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
exp_start= 08.06.2026 04:21:24.771 exp= 20.000 JD= 2461199.68165244 ap= 6.0 rotation= -4.576 *detected= 142 *matched= 137 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
exp_start= 08.06.2026 04:22:19.997 exp= 20.000 JD= 2461199.68229163 ap= 5.9 rotation= -4.568 *detected= 198 *matched= 192 status=OK /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461199.68165244
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'
Plate-solving the images
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits exists and is non-empty
NOT SAVING wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits exists and is non-empty
NOT SAVING wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits exists and is non-empty
NOT SAVING wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits exists and is non-empty
NOT SAVING wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits (1st reference image)
verification OK: wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
Image size: 937.3'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: 11:08:33.967 -01:59:30.21 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-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits (1st new image)
verification OK: wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
Image size: 941.3'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:39.859 -01:59:18.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:33.967 -01:59:30.21
Second-epoch image center 11:08:39.859 -01:59:18.08
Angular distance between the image centers 0.0248 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits (2nd new image)
verification OK: wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:37.373 -01:59:58.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:33.967 -01:59:30.21
Second-epoch image center 11:08:37.373 -01:59:58.65
Angular distance between the image centers 0.0162 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:39.859 -01:59:18.08
Second-epoch second image center 11:08:37.373 -01:59:58.65
Angular distance between the image centers 0.01530 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits &> /tmp/tmp.9TqC6pyKry
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits &> /tmp/tmp.43k3u2dynN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits &> /tmp/tmp.ozL5Xs1x0T
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits &> /tmp/tmp.gP3wPu5qZi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits and wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat
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-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits and wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat
Found non-empty wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits and wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat
The reference image (wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits) and catalog (wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat) found
'wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat' -> 'wcsmag.cat'
Read 33877 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.2320 to 175.0870 deg, Dec -7.3180 to +3.3671 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.2320 to 175.0870 deg, Dec -7.3180 to 3.3671 deg
Loaded 3877 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3086 out of 3367 total matches.
Matched with Tycho-2 3367 out of 33877 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.678150
a=0.000000 b=1.000000 c=22.678150
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 33877 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.2320 to 175.0870 deg, Dec -7.3180 to +3.3671 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.2320 to 175.0870 deg, Dec -7.3180 to 3.3671 deg
Loaded 3877 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3086 out of 3367 total matches.
Matched with Tycho-2 3367 out of 33877 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits:
Forced-photometry filter: calibrated wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits -> calib.txt_param_ref_wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits (aperture=5.0)
Read 31205 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.2881 to 175.0375 deg, Dec -7.2681 to +3.2727 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.2881 to 175.0375 deg, Dec -7.2681 to 3.2727 deg
Loaded 3807 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): 3109 out of 3359 total matches.
Matched with Tycho-2 3359 out of 31205 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits:
Forced-photometry filter: calibrated wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits -> calib.txt_param_ref_wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
2.1 pix Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
2.6 pix fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
2.5 pix fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
2.2 pix wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
2.1 pix wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
Limiting magnitude estimates:
15.3 mag. Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
15.2 mag. Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
10.6 mag. fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
11.1 mag. fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
All-image limiting magnitude estimate: 10.6 (SNR ) 10.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.9TqC6pyKry (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits' -> 'wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=1524, passed=33848
Got 33848 stars (including 32278 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat
util/solve_plate_with_UCAC5 got 33848 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 33525 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 33524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 33524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits N_match=943 sigma_overall_arcsec=0.453 sigma_q1_arcsec=0.354 sigma_q2_arcsec=0.533 sigma_q3_arcsec=0.418 sigma_q4_arcsec=0.570 n_q1=216 n_q2=238 n_q3=228 n_q4=261 worst_quadrant_to_overall_ratio=1.260
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits -region wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.43k3u2dynN (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits' -> 'wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1336, passed=31185
Got 31185 stars (including 29805 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits.cat
util/solve_plate_with_UCAC5 got 31185 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 30861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 30861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 30861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits N_match=943 sigma_overall_arcsec=0.450 sigma_q1_arcsec=0.382 sigma_q2_arcsec=0.573 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.551 n_q1=223 n_q2=227 n_q3=236 n_q4=257 worst_quadrant_to_overall_ratio=1.274
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits -region wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ozL5Xs1x0T (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_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.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_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=13, passed=1316
Got 1316 stars (including 1300 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits.cat
util/solve_plate_with_UCAC5 got 1316 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
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 469 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 906 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 906 matched stars entering correct_measured_positions(), 1234 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 469 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 1234 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 1234 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 907 stars left (next iteration limit 996)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits N_match=907 sigma_overall_arcsec=0.760 sigma_q1_arcsec=0.667 sigma_q2_arcsec=0.713 sigma_q3_arcsec=0.782 sigma_q4_arcsec=0.765 n_q1=105 n_q2=141 n_q3=320 n_q4=341 worst_quadrant_to_overall_ratio=1.028
The image catalog is written to wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits -region wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.gP3wPu5qZi (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_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.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_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=21, passed=1659
Got 1659 stars (including 1632 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits.cat
util/solve_plate_with_UCAC5 got 1659 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
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 469 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 1547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 469 (Dec -7.6 to 3.6)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 1547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 1547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits N_match=915 sigma_overall_arcsec=0.653 sigma_q1_arcsec=0.758 sigma_q2_arcsec=0.705 sigma_q3_arcsec=0.652 sigma_q4_arcsec=0.632 n_q1=91 n_q2=183 n_q3=284 n_q4=357 worst_quadrant_to_overall_ratio=1.161
The image catalog is written to wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits -region wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-21-24_20.00sec_0.00C_LIGHTs_0088.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Leo-08-Q1b1x1_234840_TTUQ1b1x1_1933478_hODzzXVx/wcs_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089.fits'
Preparing the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits at 10:48:38.12 -04:52:58.5: 11.94 +/- 0.01 detection
Forced photometry on wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits at 10:45:26.75 -04:30:45.3: 11.45 +/- 0.01 detection
Forced photometry on wcs_Leo-08-Q1b1x1_2026-04-16_00-07-23_20.00sec_-5.00C_LIGHT_0171.fits at 10:49:26.54 -05:02:00.5: 11.49 +/- 0.01 detection
Forced photometry on wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits at 10:48:38.12 -04:52:58.5: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 0.01
Forced photometry filter KEPT candidate at 10:48:38.12 -04:52:58.5: ref_mag=11.95 +/- 0.01 new_mean_mag=10.6881 delta=1.26 (need > 0.90)
Forced photometry on wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits at 10:45:26.75 -04:30:45.3: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.00
Forced photometry filter KEPT candidate at 10:45:26.75 -04:30:45.3: ref_mag=11.48 +/- 0.00 new_mean_mag=10.4139 delta=1.06 (need > 0.90)
Forced photometry on wcs_Leo-08-Q1b1x1_2026-05-10_23-15-03_20.00sec_-4.90C_LIGHT_0133.fits at 10:49:26.54 -05:02:00.5: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.01
Forced photometry filter KEPT candidate at 10:49:26.54 -05:02:00.5: ref_mag=11.52 +/- 0.01 new_mean_mag=10.4615 delta=1.06 (need > 0.90)
Adding exclusion_list_local.txt__out29283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30908.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
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 29283_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089
Preparing report for the candidate 29283_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089
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Considering the candidate 30908_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089
Preparing report for the candidate 30908_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089
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Considering the candidate 29772_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089
Preparing report for the candidate 29772_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089
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Considering the candidate 19722_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089
The candidate 19722_fd_Leo-08-Q1b1x1_2026-06-07_23-22-19_20.00sec_-0.00C_LIGHTs_0089 did not pass the final checks