This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa
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 09.4556 2461322.9556 14.25 11:05:35.33 +22:05:51.1
218.93601 65.47101 galactic Leo Second-epoch detections are separated by 2.5" and 0.4 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 | target | 11:05:35.33 +22:05:51.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:05:35.33 +22:05:51.1: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:05:35.33 +22:05:51.1: 16.28 +/- 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 09.4556* 11 05 35.33 +22 05 51.1 14.2 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
target,2461322.9556,14.25,0.05,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
target 20261009.4556 14.25CV 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 09.4556 2461322.9556 14.46 10:54:17.71 +25:49:25.2
209.07417 63.81212 galactic LMi Second-epoch detections are separated by 6.9" and 0.5 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 | target | 10:54:17.71 +25:49:25.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:54:17.71 +25:49:25.2: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:54:17.71 +25:49:25.2: 16.17 +/- 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!
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
target,2461322.9556,14.46,0.05,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
target 20261009.4556 14.46CV 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 09.4556 2461322.9556 14.09 11:19:58.74 +18:53:01.0
229.51760 67.44289 galactic Leo Second-epoch detections are separated by 5.8" and 0.4 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 | target | 11:19:58.74 +18:53:01.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:19:58.74 +18:53:01.0: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:19:58.74 +18:53:01.0: 16.09 +/- 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 09.4556* 11 19 58.74 +18 53 01.0 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461322.9556,14.09,0.05,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
target 20261009.4556 14.09CV 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 09.4556 2461322.9556 14.30 10:53:38.08 +17:55:15.9
225.45843 61.36498 galactic Leo Second-epoch detections are separated by 2.7" and 0.4 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 | target | 10:53:38.08 +17:55:15.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:53:38.08 +17:55:15.9: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:53:38.08 +17:55:15.9: 16.15 +/- 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 09.4556* 10 53 38.08 +17 55 15.9 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461322.9556,14.30,0.05,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
target 20261009.4556 14.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.4556 2461322.9556 14.51 10:47:45.38 +24:13:23.2
211.90310 62.05132 galactic LMi Second-epoch detections are separated by 6.1" and 0.4 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 | target | 10:47:45.38 +24:13:23.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:45.38 +24:13:23.2: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:45.38 +24:13:23.2: 16.18 +/- 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!
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
target,2461322.9556,14.51,0.05,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
target 20261009.4556 14.51CV 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: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
First image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Last image: 2461322.95582763 09.10.2026 10:56:13.507 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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.: -7.21
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): 5105
Objects passed selection criteria: 5065
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 3490.75
Average stars matched: 3239.75 (92.8096 %)
Memory usage VmPeak: 231472 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 10:18:29 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: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
First image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Last image: 2461322.95582763 09.10.2026 10:56:13.507 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 159
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.94
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: 9 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): 27096
Objects passed selection criteria: 26991
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: 19553.8
Average stars matched: 17829.5 (91.182 %)
Memory usage VmPeak: 249632 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 10:19:12 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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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: 2461322.95539435
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits exists and is non-empty
wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits exists and is non-empty
wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits exists and is non-empty
wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (1st reference image)
verification OK: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:04:39.891 +21:57:22.65 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits (1st new image)
verification OK: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
Image size: 941.4'x624.5' 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: 11:04:29.072 +21:56:54.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:04:39.891 +21:57:22.65
Second-epoch image center 11:04:29.072 +21:56:54.27
Angular distance between the image centers 0.0425 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits (2nd new image)
verification OK: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
Image size: 941.3'x624.5' 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: 11:04:29.056 +21:56:49.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:04:39.891 +21:57:22.65
Second-epoch image center 11:04:29.056 +21:56:49.86
Angular distance between the image centers 0.0429 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 11:04:29.072 +21:56:54.27
Second-epoch second image center 11:04:29.056 +21:56:49.86
Angular distance between the image centers 0.00123 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00123 deg. (min. required shift: 0.00164 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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits &> /tmp/tmp.nYh6KKZl1t
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits &> /tmp/tmp.xrXGjvZUsK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits &> /tmp/tmp.ObD1XAqL3r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits &> /tmp/tmp.UbrfjCqFok
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
The reference image (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits) and catalog (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat) found
'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat' -> 'wcsmag.cat'
Read 5863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6092 to 175.2053 deg, Dec +16.0209 to +27.5013 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 157.6092 to 175.2053 deg, Dec 16.0209 to 27.5013 deg
Loaded 4341 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): 3186 out of 3317 total matches.
Matched with Tycho-2 3317 out of 5863 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.852400
a=0.000000 b=1.000000 c=22.852400
From vast_summary.log: estimated ref. image limiting mag.: -7.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.64
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.64
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6092 to 175.2053 deg, Dec +16.0209 to +27.5013 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 157.6092 to 175.2053 deg, Dec 16.0209 to 27.5013 deg
Loaded 4341 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): 3186 out of 3317 total matches.
Matched with Tycho-2 3317 out of 5863 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (aperture=6.1)
Read 5873 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6047 to 175.1809 deg, Dec +16.0208 to +27.5013 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 157.6047 to 175.1809 deg, Dec 16.0208 to 27.5013 deg
Loaded 4340 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): 3163 out of 3309 total matches.
Matched with Tycho-2 3309 out of 5873 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits (aperture=6.2)
____ 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:
2.1 pix Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.1 pix Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
2.4 pix fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
2.3 pix fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
Limiting magnitude estimates:
15.6 mag. Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
15.6 mag. Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
14.3 mag. fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
14.3 mag. fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
All-image limiting magnitude estimate: 14.3 (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.nYh6KKZl1t (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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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=376, bad_region=1260, passed=5863
Got 5863 stars (including 4313 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
util/solve_plate_with_UCAC5 got 5863 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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 4123 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4116 matched stars entering correct_measured_positions(), 4116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4116 matched stars entering correct_measured_positions(), 4874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 4122 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4116 matched stars entering correct_measured_positions(), 4874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4116 matched stars entering correct_measured_positions(), 4874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4116 stars left (next iteration limit 4527)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits N_match=4116 sigma_overall_arcsec=0.288 sigma_q1_arcsec=0.272 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.254 sigma_q4_arcsec=0.294 n_q1=1255 n_q2=750 n_q3=1353 n_q4=758 worst_quadrant_to_overall_ratio=1.410
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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.xrXGjvZUsK (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-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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=393, bad_region=1276, passed=5873
Got 5873 stars (including 4297 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat
util/solve_plate_with_UCAC5 got 5873 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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 4106 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4100 matched stars entering correct_measured_positions(), 4100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4100 matched stars entering correct_measured_positions(), 4871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 4106 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4100 matched stars entering correct_measured_positions(), 4871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4100 matched stars entering correct_measured_positions(), 4871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4100 stars left (next iteration limit 4510)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits N_match=4100 sigma_overall_arcsec=0.325 sigma_q1_arcsec=0.313 sigma_q2_arcsec=0.454 sigma_q3_arcsec=0.298 sigma_q4_arcsec=0.312 n_q1=1228 n_q2=741 n_q3=1368 n_q4=763 worst_quadrant_to_overall_ratio=1.396
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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.ObD1XAqL3r (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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
Checking if the catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
WCS catalog name: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.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=179, bad_region=466, passed=2935
Got 2935 stars (including 2311 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat
util/solve_plate_with_UCAC5 got 2935 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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 2168 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2162 matched stars entering correct_measured_positions(), 2162 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2162 matched stars entering correct_measured_positions(), 2546 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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 2168 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2162 matched stars entering correct_measured_positions(), 2546 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 2162 matched stars entering correct_measured_positions(), 2547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 2162 stars left (next iteration limit 2378)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2162 robust_rms=6.481 arcsec worst_region_rms=11.613 arcsec outer_annulus_rms=11.613 arcsec
SIP_REFIT: SIP order 3 trial: matched=2162 robust_rms=0.567 arcsec worst_region_rms=0.731 arcsec outer_annulus_rms=0.555 arcsec
SIP_REFIT: SIP order 5 trial: matched=2162 robust_rms=0.437 arcsec worst_region_rms=0.506 arcsec outer_annulus_rms=0.465 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2162 robust_rms_before=2.025 arcsec robust_rms_before_corrected=0.398 arcsec robust_rms_after=0.437 arcsec worst_region_rms_before=0.486 worst_region_rms_after=0.506 outer_annulus_rms_before=1.649 outer_annulus_rms_after=0.465
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.486 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits worst_region_rms_kept=0.486 arcsec robust_rms_kept=0.398 arcsec matched=2162
WCS_QUALITY_DIAG: file=fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits N_match=2162 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.388 sigma_q2_arcsec=0.448 sigma_q3_arcsec=0.391 sigma_q4_arcsec=0.417 n_q1=742 n_q2=338 n_q3=715 n_q4=367 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits -region wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.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.UbrfjCqFok (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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
Checking if the catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
WCS catalog name: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=180, bad_region=475, passed=2879
Got 2879 stars (including 2253 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat
util/solve_plate_with_UCAC5 got 2879 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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 2112 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2107 matched stars entering correct_measured_positions(), 2107 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2107 matched stars entering correct_measured_positions(), 2484 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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 2114 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2110 matched stars entering correct_measured_positions(), 2484 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 2110 matched stars entering correct_measured_positions(), 2484 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 2110 stars left (next iteration limit 2317)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2110 robust_rms=6.513 arcsec worst_region_rms=13.030 arcsec outer_annulus_rms=13.030 arcsec
SIP_REFIT: SIP order 3 trial: matched=2110 robust_rms=0.557 arcsec worst_region_rms=0.636 arcsec outer_annulus_rms=0.547 arcsec
SIP_REFIT: SIP order 5 trial: matched=2110 robust_rms=0.417 arcsec worst_region_rms=0.480 arcsec outer_annulus_rms=0.480 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2110 robust_rms_before=1.862 arcsec robust_rms_before_corrected=0.410 arcsec robust_rms_after=0.417 arcsec worst_region_rms_before=0.485 worst_region_rms_after=0.480 outer_annulus_rms_before=1.476 outer_annulus_rms_after=0.480
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.485 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits worst_region_rms_kept=0.485 arcsec robust_rms_kept=0.410 arcsec matched=2110
WCS_QUALITY_DIAG: file=fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits N_match=2110 sigma_overall_arcsec=0.435 sigma_q1_arcsec=0.372 sigma_q2_arcsec=0.464 sigma_q3_arcsec=0.441 sigma_q4_arcsec=0.472 n_q1=712 n_q2=340 n_q3=697 n_q4=361 worst_quadrant_to_overall_ratio=1.087
The image catalog is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits -region wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
Saving the final (post-refit) wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits'
Saving the final (post-refit) wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits to local_wcs_cache/
'wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits' -> 'local_wcs_cache/wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits'
Saving the final (post-refit) wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits to local_wcs_cache/
'wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits' -> 'local_wcs_cache/wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits sigma_overall=0.288 worst_q_ratio=1.410
ref2=Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits sigma_overall=0.325 worst_q_ratio=1.396
new1=fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits sigma_overall=0.405 worst_q_ratio=1.107
new2=fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits sigma_overall=0.435 worst_q_ratio=1.087
reference average sigma_overall=0.3065 worst_q_ratio=1.403
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176_astrometric_residuals.png (4116 matched stars from wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177_astrometric_residuals.png (4100 matched stars from wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598_astrometric_residuals.png (2162 matched stars from wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599_astrometric_residuals.png (2110 matched stars from wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits'
Saving fully-calibrated image wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits'
Preparing the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Leo-03-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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits exists and is non-empty
wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits exists and is non-empty
wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits exists and is non-empty
wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (1st reference image)
verification OK: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Image size: 941.4'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:04:39.891 +21:57:22.65 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits (1st new image)
verification OK: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
Image size: 941.4'x624.5' 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: 11:04:29.072 +21:56:54.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:04:39.891 +21:57:22.65
Second-epoch image center 11:04:29.072 +21:56:54.27
Angular distance between the image centers 0.0425 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits (2nd new image)
verification OK: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
Image size: 941.3'x624.5' 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: 11:04:29.056 +21:56:49.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:04:39.891 +21:57:22.65
Second-epoch image center 11:04:29.056 +21:56:49.86
Angular distance between the image centers 0.0429 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 11:04:29.072 +21:56:54.27
Second-epoch second image center 11:04:29.056 +21:56:49.86
Angular distance between the image centers 0.00123 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00123 deg. (min. required shift: 0.00164 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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits &> /tmp/tmp.tiaOQDUyy9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits &> /tmp/tmp.CP9D5aAyvX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits &> /tmp/tmp.3pET51RbUp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits &> /tmp/tmp.ezzaXNn3FC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
The reference image (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits) and catalog (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat) found
'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat' -> 'wcsmag.cat'
Read 31701 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6088 to 175.2809 deg, Dec +16.0209 to +27.5079 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 157.6088 to 175.2809 deg, Dec 16.0209 to 27.5079 deg
Loaded 4356 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): 3099 out of 3355 total matches.
Matched with Tycho-2 3355 out of 31701 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.749200
a=0.000000 b=1.000000 c=22.749200
From vast_summary.log: estimated ref. image limiting mag.: -6.94
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.81
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.81
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31701 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6088 to 175.2809 deg, Dec +16.0209 to +27.5079 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 157.6088 to 175.2809 deg, Dec 16.0209 to 27.5079 deg
Loaded 4356 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): 3099 out of 3355 total matches.
Matched with Tycho-2 3355 out of 31701 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (aperture=4.8)
Read 31604 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.5934 to 175.2806 deg, Dec +16.0208 to +27.5110 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 157.5934 to 175.2806 deg, Dec 16.0208 to 27.5110 deg
Loaded 4365 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): 3074 out of 3356 total matches.
Matched with Tycho-2 3356 out of 31604 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 119 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.0 pix Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
2.3 pix fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
2.2 pix fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
Limiting magnitude estimates:
15.8 mag. Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
15.8 mag. Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
14.5 mag. fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
14.6 mag. fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 13.9 (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.tiaOQDUyy9 (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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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=10, blended=1119, bad_region=6774, passed=31691
Got 31691 stars (including 24018 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
util/solve_plate_with_UCAC5 got 31691 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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 4776 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 4772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 26442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 4776 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 26442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 26442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4772 stars left (next iteration limit 5249)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits N_match=4772 sigma_overall_arcsec=0.288 sigma_q1_arcsec=0.272 sigma_q2_arcsec=0.396 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.280 n_q1=1457 n_q2=932 n_q3=1519 n_q4=864 worst_quadrant_to_overall_ratio=1.377
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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.CP9D5aAyvX (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-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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=1160, bad_region=6772, passed=31589
Got 31589 stars (including 23891 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat
util/solve_plate_with_UCAC5 got 31589 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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 4777 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4773 matched stars entering correct_measured_positions(), 4773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4773 matched stars entering correct_measured_positions(), 26332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 4777 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4773 matched stars entering correct_measured_positions(), 26332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4773 matched stars entering correct_measured_positions(), 26332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4773 stars left (next iteration limit 5250)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits N_match=4773 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.305 sigma_q2_arcsec=0.451 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.315 n_q1=1443 n_q2=931 n_q3=1520 n_q4=879 worst_quadrant_to_overall_ratio=1.403
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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.3pET51RbUp (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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
Checking if the catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
WCS catalog name: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.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=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=824, bad_region=2094, passed=16722
Got 16722 stars (including 13923 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat
util/solve_plate_with_UCAC5 got 16722 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 532 to 588 (Dec 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 4661 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4654 matched stars entering correct_measured_positions(), 4655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4654 matched stars entering correct_measured_positions(), 15214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 532 to 588 (Dec 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 4662 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4657 matched stars entering correct_measured_positions(), 15214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4657 matched stars entering correct_measured_positions(), 15214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4657 stars left (next iteration limit 5119)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.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=4657 robust_rms=6.519 arcsec worst_region_rms=12.587 arcsec outer_annulus_rms=12.587 arcsec
SIP_REFIT: SIP order 3 trial: matched=4657 robust_rms=0.608 arcsec worst_region_rms=0.833 arcsec outer_annulus_rms=0.632 arcsec
SIP_REFIT: SIP order 5 trial: matched=4657 robust_rms=0.494 arcsec worst_region_rms=0.579 arcsec outer_annulus_rms=0.559 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4657 robust_rms_before=2.081 arcsec robust_rms_before_corrected=0.437 arcsec robust_rms_after=0.494 arcsec worst_region_rms_before=0.568 worst_region_rms_after=0.579 outer_annulus_rms_before=1.737 outer_annulus_rms_after=0.559
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.568 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits worst_region_rms_kept=0.568 arcsec robust_rms_kept=0.437 arcsec matched=4657
WCS_QUALITY_DIAG: file=fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits N_match=4657 sigma_overall_arcsec=0.434 sigma_q1_arcsec=0.422 sigma_q2_arcsec=0.532 sigma_q3_arcsec=0.407 sigma_q4_arcsec=0.435 n_q1=1515 n_q2=701 n_q3=1651 n_q4=790 worst_quadrant_to_overall_ratio=1.225
The image catalog is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits -region wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.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.ezzaXNn3FC (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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
Checking if the catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat corresponding to the image wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
WCS catalog name: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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=1, blended=692, bad_region=2217, passed=16682
Got 16682 stars (including 14018 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat
util/solve_plate_with_UCAC5 got 16682 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 532 to 588 (Dec 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 4662 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4656 matched stars entering correct_measured_positions(), 4656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4656 matched stars entering correct_measured_positions(), 15056 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 532 to 588 (Dec 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 4663 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 15056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4658 matched stars entering correct_measured_positions(), 15057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4658 stars left (next iteration limit 5121)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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=4658 robust_rms=6.510 arcsec worst_region_rms=12.827 arcsec outer_annulus_rms=12.827 arcsec
SIP_REFIT: SIP order 3 trial: matched=4658 robust_rms=0.587 arcsec worst_region_rms=0.718 arcsec outer_annulus_rms=0.616 arcsec
SIP_REFIT: SIP order 5 trial: matched=4658 robust_rms=0.469 arcsec worst_region_rms=0.576 arcsec outer_annulus_rms=0.576 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4658 robust_rms_before=1.908 arcsec robust_rms_before_corrected=0.429 arcsec robust_rms_after=0.469 arcsec worst_region_rms_before=0.504 worst_region_rms_after=0.576 outer_annulus_rms_before=1.579 outer_annulus_rms_after=0.576
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.504 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits worst_region_rms_kept=0.504 arcsec robust_rms_kept=0.429 arcsec matched=4658
WCS_QUALITY_DIAG: file=fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits N_match=4658 sigma_overall_arcsec=0.441 sigma_q1_arcsec=0.413 sigma_q2_arcsec=0.508 sigma_q3_arcsec=0.442 sigma_q4_arcsec=0.442 n_q1=1505 n_q2=701 n_q3=1653 n_q4=799 worst_quadrant_to_overall_ratio=1.151
The image catalog is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Leo-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits -region wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-55-36_20.00sec_0.00C_LIGHT_0598.fits
Saving fully-calibrated image wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.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-03-Q2b1x1_101600_TTUQ2b1x1_2616848_5txdMKKa/wcs_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599.fits
Preparing the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:05:35.33 +22:05:51.1: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:19:58.74 +18:53:01.0: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:53:38.08 +17:55:15.9: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:54:17.71 +25:49:25.2: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:45.38 +24:13:23.2: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:05:35.33 +22:05:51.1: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:19:58.74 +18:53:01.0: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:53:38.08 +17:55:15.9: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:54:17.71 +25:49:25.2: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:45.38 +24:13:23.2: 16.18 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out56333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56474.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 51933_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 51933_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 51985_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 51985_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52148_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52148_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52377_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52377_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52528_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52528_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52599_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52599_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52702_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52702_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52787_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52787_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52825_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52825_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52847_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52847_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52853_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52853_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52912_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52912_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52915_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52915_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52933_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52933_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52935_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52935_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52968_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52968_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
**** FOUND 10:55:27.54 +24:43:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52990_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 52990_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53072_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53072_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53084_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53084_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53177_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53177_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53200_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53200_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53245_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53245_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53276_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53276_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53277_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53277_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53298_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53298_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53418_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53418_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53420_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53420_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53461_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53461_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53521_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53521_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53539_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53539_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53561_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53561_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53571_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53571_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53583_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53583_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53595_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53595_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53610_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53610_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53638_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53638_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53700_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53700_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53736_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53736_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53764_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53764_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53775_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53775_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
**** FOUND 11:08:42.04 +24:38:45.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53798_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53798_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
**** FOUND 11:02:28.57 +20:10:47.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53832_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53832_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53848_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53848_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53902_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 53902_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54066_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54066_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54090_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54090_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54194_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54194_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54240_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54240_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54360_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54360_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54445_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54445_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54455_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54455_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54501_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54501_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54502_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54502_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
**** FOUND 10:46:35.54 +24:40:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54595_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54595_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54676_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54676_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54707_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54707_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
**** FOUND 11:13:34.14 +20:06:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54880_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54880_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54930_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54930_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54972_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54972_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54975_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 54975_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55074_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55074_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55139_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55139_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55186_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55186_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55188_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55188_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55202_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55202_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55236_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55236_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55240_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55240_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55243_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55243_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55249_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55249_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55299_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55299_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55396_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55396_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55406_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55406_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55424_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55424_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55433_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55433_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55473_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55473_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55480_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55480_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55529_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55529_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55557_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55557_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55601_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55601_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55618_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55618_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55637_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55637_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55675_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55675_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55707_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55707_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55709_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55709_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55747_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55747_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55754_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55754_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55837_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55837_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55838_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55838_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55872_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55872_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55944_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55944_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55970_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55970_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55980_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55980_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55987_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 55987_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56032_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56032_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56035_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56035_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56043_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56043_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56090_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56090_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56125_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56125_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56141_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56141_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56172_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56172_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56197_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56197_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56234_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56234_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56238_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56238_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56250_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56250_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56279_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56279_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56333_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
Preparing report for the candidate 56333_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
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Considering the candidate 56345_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56345_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56356_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56356_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56362_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56362_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56364_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56364_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56376_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56376_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56409_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
Preparing report for the candidate 56409_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
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Considering the candidate 56413_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56413_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56442_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
Preparing report for the candidate 56442_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
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Considering the candidate 56456_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
Preparing report for the candidate 56456_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
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Considering the candidate 56473_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56473_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56474_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
Preparing report for the candidate 56474_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
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Considering the candidate 56477_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56477_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56492_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599
The candidate 56492_fd_Leo-03-Q2b1x1_2026-10-09_05-56-13_20.00sec_-0.00C_LIGHT_0599 did not pass the final checks
