This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 14.1877 2461205.6877 12.13 10:12:26.74 +10:53:57.9
228.58898 49.30184 galactic Leo Second-epoch detections are separated by 0.9" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.41 Daphne 0 -0 0 12.3 -0 0
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:12:26.74 +10:53:57.9: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:12:26.74 +10:53:57.9: 15.70 +/- 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 06 14.1877* 10 12 26.74 +10 53 57.9 12.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461205.6877,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260614.1877 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1877 2461205.6877 12.20 10:46:04.18 +11:50:07.2
234.24604 56.87510 galactic Leo Second-epoch detections are separated by 0.5" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.11 Parthenope 0 -0 0 12.0 -0 0
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:46:04.18 +11:50:07.2: 15.81 +/- 0.34 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:46:04.18 +11:50:07.2: 15.86 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.81 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1877* 10 46 04.18 +11 50 07.2 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461205.6877,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260614.1877 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1877 2461205.6877 13.04 10:58:27.82 +17:55:10.2
226.46546 62.41111 galactic Leo Second-epoch detections are separated by 0.8" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.416 Vaticana -0 -0 0 12.9 0 -0
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:58:27.82 +17:55:10.2: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:58:27.82 +17:55:10.2: 15.84 +/- 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 06 14.1877* 10 58 27.82 +17 55 10.2 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461205.6877,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260614.1877 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1877 2461205.6877 13.23 10:26:23.54 +13:05:04.4
228.14268 53.34257 galactic Leo Second-epoch detections are separated by 0.7" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.103 Hera 0 -0 0 13.4 -0 0
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:26:23.54 +13:05:04.4: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:26:23.54 +13:05:04.4: 15.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 14.1877* 10 26 23.54 +13 05 04.4 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461205.6877,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260614.1877 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1877 2461205.6877 13.90 10:09:36.85 +12:42:09.3
225.64227 49.54257 galactic Leo Second-epoch detections are separated by 0.6" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.47 Aglaja 0 0 0 14.3 0 -0
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:09:36.85 +12:42:09.3: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:09:36.85 +12:42:09.3: 15.74 +/- 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 06 14.1877* 10 09 36.85 +12 42 09.3 13.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461205.6877,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260614.1877 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 14.1877 2461205.6877 14.53 10:51:12.80 +17:47:02.0
225.23186 60.78291 galactic Leo Second-epoch detections are separated by 0.3" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.508 Princetonia -0 0 0 14.4 -0 0
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:51:12.80 +17:47:02.0: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:51:12.80 +17:47:02.0: 15.84 +/- 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 06 14.1877* 10 51 12.80 +17 47 02.0 14.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461205.6877,14.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260614.1877 14.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461171.68283635 11.05.2026 04:23:07.061 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
First image: 2461171.68283635 11.05.2026 04:23:07.061 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Last image: 2461205.68798626 14.06.2026 04:30:32.013 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5531
Objects passed selection criteria: 5513
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 4237.25
Average stars matched: 4154.5 (98.0471 %)
Memory usage VmPeak: 111624 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jun 13 23:37:37 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461171.68283635 11.05.2026 04:23:07.061 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
First image: 2461171.68283635 11.05.2026 04:23:07.061 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Last image: 2461205.68798626 14.06.2026 04:30:32.013 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 30
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 10 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 27824
Objects passed selection criteria: 27737
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 23685.2
Average stars matched: 22824.2 (96.3648 %)
Memory usage VmPeak: 131048 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jun 13 23:39:05 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
SExtractor catalog cache: saved Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.cat to cache
SExtractor catalog cache: saved Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461205.68746940
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits exists and is non-empty
Saving wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits to local_wcs_cache/
'wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits' -> 'local_wcs_cache/wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits'
wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits exists and is non-empty
Saving wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits to local_wcs_cache/
'wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits' -> 'local_wcs_cache/wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits'
wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits exists and is non-empty
Saving wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits to local_wcs_cache/
'wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits' -> 'local_wcs_cache/wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits'
wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits exists and is non-empty
Saving wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits to local_wcs_cache/
'wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits' -> 'local_wcs_cache/wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits (1st reference image)
verification OK: wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:40:00.126 +14:00:12.98 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits (1st new image)
verification OK: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
Image size: 941.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:40:05.956 +13:59:29.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:40:00.126 +14:00:12.98
Second-epoch image center 10:40:05.956 +13:59:29.24
Angular distance between the image centers 0.0265 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits (2nd new image)
verification OK: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
Image size: 941.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:40:03.336 +13:58:49.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:40:00.126 +14:00:12.98
Second-epoch image center 10:40:03.336 +13:58:49.13
Angular distance between the image centers 0.0267 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:40:05.956 +13:59:29.24
Second-epoch second image center 10:40:03.336 +13:58:49.13
Angular distance between the image centers 0.01537 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits &> /tmp/tmp.rUayF2Wp4k
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits &> /tmp/tmp.mY1mHbwN9v
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits &> /tmp/tmp.dagvPD94m9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits &> /tmp/tmp.FwUEJBHrK6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
Found non-empty wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
The reference image (wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits) and catalog (wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat) found
'wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat' -> 'wcsmag.cat'
Read 5744 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7234 to 168.1820 deg, Dec +8.6409 to +19.2606 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.7234 to 168.1820 deg, Dec 8.6409 to 19.2606 deg
Loaded 4238 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): 3433 out of 3512 total matches.
Matched with Tycho-2 3512 out of 5744 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.729100
a=0.000000 b=1.000000 c=22.729100
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.12
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.12
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5744 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7234 to 168.1820 deg, Dec +8.6409 to +19.2606 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.7234 to 168.1820 deg, Dec 8.6409 to 19.2606 deg
Loaded 4238 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): 3433 out of 3512 total matches.
Matched with Tycho-2 3512 out of 5744 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits:
Forced-photometry filter: calibrated wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits -> calib.txt_param_ref_wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits (aperture=6.6)
Read 5709 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7044 to 168.1822 deg, Dec +8.6409 to +19.2438 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.7044 to 168.1822 deg, Dec 8.6409 to 19.2438 deg
Loaded 4241 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): 3438 out of 3510 total matches.
Matched with Tycho-2 3510 out of 5709 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits:
Forced-photometry filter: calibrated wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits -> calib.txt_param_ref_wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
2.4 pix Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
2.2 pix fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
2.2 pix fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
2.4 pix wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
2.4 pix wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Limiting magnitude estimates:
15.1 mag. Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
15.1 mag. Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
14.2 mag. fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
14.1 mag. fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.rUayF2Wp4k (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-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.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-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits' -> 'wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS-calibrated image found: wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Checking if the catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat corresponding to the image wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat corresponding to the image wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS catalog name: wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=319, passed=5744
Got 5744 stars (including 5420 good ones) from the SExtractor catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
util/solve_plate_with_UCAC5 got 5744 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 5652 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
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 5650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 869 matched stars entering correct_measured_positions(), 5650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 869 stars left (next iteration limit 955)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits N_match=869 sigma_overall_arcsec=0.444 sigma_q1_arcsec=0.358 sigma_q2_arcsec=0.485 sigma_q3_arcsec=0.386 sigma_q4_arcsec=0.590 n_q1=198 n_q2=228 n_q3=236 n_q4=207 worst_quadrant_to_overall_ratio=1.329
The image catalog is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits -region wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.mY1mHbwN9v (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-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.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-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits' -> 'wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS-calibrated image found: wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Checking if the catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS catalog name: wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=309, passed=5709
Got 5709 stars (including 5396 good ones) from the SExtractor catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat
util/solve_plate_with_UCAC5 got 5709 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.2)
Done reading UCAC5 zone files...
Matched 865 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 865 matched stars entering correct_measured_positions(), 852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 865 matched stars entering correct_measured_positions(), 5614 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.2)
Done reading UCAC5 zone files...
Matched 865 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 865 matched stars entering correct_measured_positions(), 5612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 865 matched stars entering correct_measured_positions(), 5612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 865 stars left (next iteration limit 951)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits N_match=865 sigma_overall_arcsec=0.437 sigma_q1_arcsec=0.308 sigma_q2_arcsec=0.516 sigma_q3_arcsec=0.391 sigma_q4_arcsec=0.571 n_q1=197 n_q2=222 n_q3=239 n_q4=207 worst_quadrant_to_overall_ratio=1.307
The image catalog is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits -region wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dagvPD94m9 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
Checking if the catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
WCS catalog name: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=170, passed=2827
Got 2827 stars (including 2655 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat
util/solve_plate_with_UCAC5 got 2827 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 862 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 862 matched stars entering correct_measured_positions(), 837 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 862 matched stars entering correct_measured_positions(), 2724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 862 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 862 matched stars entering correct_measured_positions(), 2727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 862 matched stars entering correct_measured_positions(), 2727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 862 stars left (next iteration limit 948)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits N_match=862 sigma_overall_arcsec=0.338 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.312 sigma_q4_arcsec=0.318 n_q1=220 n_q2=268 n_q3=183 n_q4=191 worst_quadrant_to_overall_ratio=1.006
The image catalog is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits -region wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FwUEJBHrK6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
Checking if the catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
WCS catalog name: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=157, passed=2765
Got 2765 stars (including 2603 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat
util/solve_plate_with_UCAC5 got 2765 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 863 matched stars entering correct_measured_positions(), 841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 863 matched stars entering correct_measured_positions(), 2670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 863 matched stars entering correct_measured_positions(), 2669 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 863 matched stars entering correct_measured_positions(), 2669 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 863 stars left (next iteration limit 949)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits N_match=863 sigma_overall_arcsec=0.339 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.353 sigma_q3_arcsec=0.321 sigma_q4_arcsec=0.347 n_q1=223 n_q2=264 n_q3=190 n_q4=186 worst_quadrant_to_overall_ratio=1.042
The image catalog is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits -region wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits sigma_overall=0.444 worst_q_ratio=1.329
ref2=Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits sigma_overall=0.437 worst_q_ratio=1.307
new1=fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits sigma_overall=0.338 worst_q_ratio=1.006
new2=fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits sigma_overall=0.339 worst_q_ratio=1.042
reference average sigma_overall=0.4405 worst_q_ratio=1.318
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141_astrometric_residuals.png (869 matched stars from wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142_astrometric_residuals.png (865 matched stars from wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074_astrometric_residuals.png (862 matched stars from wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075_astrometric_residuals.png (863 matched stars from wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits'
Saving fully-calibrated image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits'
Preparing the HTML report for the field Leo-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:15:12.03 +11:41:08.1: 10.94 +/- 0.01 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:15:12.03 +11:41:08.1: 10.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.00
Forced photometry filter REJECTED candidate at 10:15:12.03 +11:41:08.1: ref_mag=10.95 +/- 0.00 new_mean_mag=11.1465 delta=-0.20 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20287_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 20287_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Leo-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
SExtractor catalog cache: saved Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.cat to cache
SExtractor catalog cache: saved Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Creating symlink local_wcs_cache/wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits exists and is non-empty
wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits exists and is non-empty
wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits exists and is non-empty
wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits (1st reference image)
verification OK: wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:40:00.126 +14:00:12.98 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits (1st new image)
verification OK: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
Image size: 941.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:40:05.956 +13:59:29.24 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:40:00.126 +14:00:12.98
Second-epoch image center 10:40:05.956 +13:59:29.24
Angular distance between the image centers 0.0265 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits (2nd new image)
verification OK: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
Image size: 941.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:40:03.336 +13:58:49.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:40:00.126 +14:00:12.98
Second-epoch image center 10:40:03.336 +13:58:49.13
Angular distance between the image centers 0.0267 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:40:05.956 +13:59:29.24
Second-epoch second image center 10:40:03.336 +13:58:49.13
Angular distance between the image centers 0.01537 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits &> /tmp/tmp.5SxvZDiKZe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits &> /tmp/tmp.zoMXl5L7zZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits &> /tmp/tmp.TppqCsPmbO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits &> /tmp/tmp.G5I7rkQWLI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
Found non-empty wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits and wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
The reference image (wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits) and catalog (wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat) found
'wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat' -> 'wcsmag.cat'
Read 29548 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7133 to 168.2349 deg, Dec +8.6409 to +19.2695 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.7133 to 168.2349 deg, Dec 8.6409 to 19.2695 deg
Loaded 4250 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3395 out of 3603 total matches.
Matched with Tycho-2 3603 out of 29548 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.606600
a=0.000000 b=1.000000 c=22.606600
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29548 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7133 to 168.2349 deg, Dec +8.6409 to +19.2695 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.7133 to 168.2349 deg, Dec 8.6409 to 19.2695 deg
Loaded 4250 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3395 out of 3603 total matches.
Matched with Tycho-2 3603 out of 29548 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits:
Forced-photometry filter: calibrated wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits -> calib.txt_param_ref_wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits (aperture=5.1)
Read 29453 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 151.7044 to 168.1930 deg, Dec +8.6409 to +19.2613 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 151.7044 to 168.1930 deg, Dec 8.6409 to 19.2613 deg
Loaded 4244 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): 3391 out of 3603 total matches.
Matched with Tycho-2 3603 out of 29453 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits:
Forced-photometry filter: calibrated wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits -> calib.txt_param_ref_wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
2.2 pix Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
2.0 pix fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
2.1 pix fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
2.2 pix wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
2.2 pix wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Limiting magnitude estimates:
15.3 mag. Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
15.3 mag. Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
14.4 mag. fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
14.4 mag. fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
All-image limiting magnitude estimate: 14.4 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5SxvZDiKZe (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-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.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-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits' -> 'wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS-calibrated image found: wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
Checking if the catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat corresponding to the image wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat corresponding to the image wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits
WCS catalog name: wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=1176, passed=29525
Got 29525 stars (including 28308 good ones) from the SExtractor catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat
util/solve_plate_with_UCAC5 got 29525 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 29072 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
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 29072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 870 matched stars entering correct_measured_positions(), 29072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 870 stars left (next iteration limit 957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits N_match=870 sigma_overall_arcsec=0.441 sigma_q1_arcsec=0.383 sigma_q2_arcsec=0.457 sigma_q3_arcsec=0.376 sigma_q4_arcsec=0.582 n_q1=205 n_q2=228 n_q3=235 n_q4=202 worst_quadrant_to_overall_ratio=1.321
The image catalog is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits -region wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zoMXl5L7zZ (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-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.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-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits' -> 'wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS-calibrated image found: wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
Checking if the catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits
WCS catalog name: wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1170, passed=29431
Got 29431 stars (including 28231 good ones) from the SExtractor catalog wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat
util/solve_plate_with_UCAC5 got 29431 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 871 matched stars entering correct_measured_positions(), 860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 871 matched stars entering correct_measured_positions(), 28987 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
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 871 matched stars entering correct_measured_positions(), 28986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 871 matched stars entering correct_measured_positions(), 28986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 871 stars left (next iteration limit 958)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits N_match=871 sigma_overall_arcsec=0.457 sigma_q1_arcsec=0.336 sigma_q2_arcsec=0.534 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.552 n_q1=201 n_q2=225 n_q3=239 n_q4=206 worst_quadrant_to_overall_ratio=1.207
The image catalog is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits -region wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TppqCsPmbO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
Checking if the catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
WCS catalog name: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=430, passed=18351
Got 18351 stars (including 17885 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat
util/solve_plate_with_UCAC5 got 18351 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 861 matched stars entering correct_measured_positions(), 838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 861 matched stars entering correct_measured_positions(), 17640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 861 matched stars entering correct_measured_positions(), 17643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 861 matched stars entering correct_measured_positions(), 17643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 861 stars left (next iteration limit 947)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits N_match=861 sigma_overall_arcsec=0.330 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.343 sigma_q3_arcsec=0.311 sigma_q4_arcsec=0.321 n_q1=225 n_q2=265 n_q3=183 n_q4=188 worst_quadrant_to_overall_ratio=1.037
The image catalog is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits -region wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.G5I7rkQWLI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
Checking if the catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
WCS catalog name: wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=602, passed=18338
Got 18338 stars (including 17697 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat
util/solve_plate_with_UCAC5 got 18338 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 863 matched stars entering correct_measured_positions(), 847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 863 matched stars entering correct_measured_positions(), 17613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 863 matched stars entering correct_measured_positions(), 17613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 863 matched stars entering correct_measured_positions(), 17613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 863 stars left (next iteration limit 949)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits N_match=863 sigma_overall_arcsec=0.336 sigma_q1_arcsec=0.316 sigma_q2_arcsec=0.345 sigma_q3_arcsec=0.313 sigma_q4_arcsec=0.344 n_q1=224 n_q2=263 n_q3=191 n_q4=185 worst_quadrant_to_overall_ratio=1.027
The image catalog is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits -region wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.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_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-29-47_20.00sec_-0.00C_LIGHTs_0074.fits
Saving fully-calibrated image wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.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_2026-06-13_CI_Leo-05-Q1b1x1_233526_TTUQ1b1x1_2987582_YdDnGunU/wcs_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075.fits
Preparing the HTML report for the field Leo-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:08:21.10 +13:58:14.1: 13.56 +/- 0.05 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:15:12.04 +11:41:08.5: 11.11 +/- 0.01 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:46:04.18 +11:50:07.2: 15.81 +/- 0.34 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:12:26.74 +10:53:57.9: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:31:01.71 +17:50:08.6: 12.18 +/- 0.01 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:45:44.66 +16:24:44.0: 12.28 +/- 0.01 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:14:14.68 +14:09:35.2: 12.11 +/- 0.01 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:42:35.21 +13:25:48.3: 12.65 +/- 0.02 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:20:28.37 +10:06:24.4: 11.94 +/- 0.01 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:58:27.82 +17:55:10.2: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:12:26.74 +10:53:57.9: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:31:01.71 +17:50:08.6: 12.19 +/- 0.01 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:15:12.04 +11:41:08.5: 11.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry reference-image weighted average: 11.12 +/- 0.00
Forced photometry filter REJECTED candidate at 10:31:01.71 +17:50:08.6: ref_mag=12.18 +/- 0.01 new_mean_mag=12.4755 delta=-0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:15:12.04 +11:41:08.5: ref_mag=11.12 +/- 0.00 new_mean_mag=11.1740 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:08:21.10 +13:58:14.1: 13.50 +/- 0.05 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:45:44.66 +16:24:44.0: 12.22 +/- 0.01 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:46:04.18 +11:50:07.2: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:42:35.21 +13:25:48.3: 12.60 +/- 0.02 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:14:14.68 +14:09:35.2: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Forced photometry reference-image weighted average: 15.81 +/- 0.34
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter REJECTED candidate at 10:08:21.10 +13:58:14.1: ref_mag=13.53 +/- 0.03 new_mean_mag=13.5980 delta=-0.07 (need > 0.90)
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter KEPT candidate at 10:46:04.18 +11:50:07.2: ref_mag=15.81 +/- 0.34 new_mean_mag=12.1957 delta=3.62 (need > 0.90)
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry filter REJECTED candidate at 10:45:44.66 +16:24:44.0: ref_mag=12.25 +/- 0.01 new_mean_mag=12.8172 delta=-0.57 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:42:35.21 +13:25:48.3: ref_mag=12.63 +/- 0.01 new_mean_mag=13.2038 delta=-0.58 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:14:14.68 +14:09:35.2: ref_mag=12.08 +/- 0.01 new_mean_mag=12.3325 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:20:28.37 +10:06:24.4: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:58:27.82 +17:55:10.2: 15.84 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 10:20:28.37 +10:06:24.4: ref_mag=11.93 +/- 0.01 new_mean_mag=12.2539 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:26:23.54 +13:05:04.4: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:37:37.37 +15:03:56.8: 12.73 +/- 0.02 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:20:56.01 +12:29:13.8: 12.99 +/- 0.03 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:12:30.46 +17:24:38.8: 13.57 +/- 0.05 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:08:50.83 +18:59:21.1: 14.38 +/- 0.11 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:09:36.85 +12:42:09.3: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:26:23.54 +13:05:04.4: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:20:56.01 +12:29:13.8: 12.99 +/- 0.03 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:09:43.97 +18:06:00.1: 14.72 +/- 0.15 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:37:37.37 +15:03:56.8: 12.71 +/- 0.02 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:12:30.46 +17:24:38.8: 13.73 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter REJECTED candidate at 10:20:56.01 +12:29:13.8: ref_mag=12.99 +/- 0.02 new_mean_mag=13.2338 delta=-0.25 (need > 0.90)
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Forced photometry filter REJECTED candidate at 10:37:37.37 +15:03:56.8: ref_mag=12.72 +/- 0.01 new_mean_mag=13.0781 delta=-0.36 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:12:30.46 +17:24:38.8: ref_mag=13.64 +/- 0.04 new_mean_mag=13.6924 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:08:50.83 +18:59:21.1: 14.44 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.08
Forced photometry filter REJECTED candidate at 10:08:50.83 +18:59:21.1: ref_mag=14.41 +/- 0.08 new_mean_mag=14.1373 delta=0.27 (need > 0.90)
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:09:36.85 +12:42:09.3: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:09:43.97 +18:06:00.1: 14.59 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.10
Forced photometry filter REJECTED candidate at 10:09:43.97 +18:06:00.1: ref_mag=14.65 +/- 0.10 new_mean_mag=13.9872 delta=0.66 (need > 0.90)
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:09:44.00 +17:40:41.2: 14.52 +/- 0.12 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:08:30.00 +14:07:53.4: 14.69 +/- 0.14 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-23-07_20.00sec_-5.00C_LIGHT_0141.fits at 10:51:12.80 +17:47:02.0: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:08:30.00 +14:07:53.4: 14.76 +/- 0.15 detection
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:09:44.00 +17:40:41.2: 14.57 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.10
Forced photometry reference-image weighted average: 14.54 +/- 0.08
Forced photometry filter REJECTED candidate at 10:08:30.00 +14:07:53.4: ref_mag=14.72 +/- 0.10 new_mean_mag=13.8664 delta=0.85 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:09:44.00 +17:40:41.2: ref_mag=14.54 +/- 0.08 new_mean_mag=14.3434 delta=0.20 (need > 0.90)
Forced photometry on wcs_Leo-05-Q1b1x1_2026-05-10_23-24-02_20.00sec_-4.90C_LIGHT_0142.fits at 10:51:12.80 +17:47:02.0: 15.84 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out32321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32965.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 32158_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32158_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32159_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32159_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32160_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32160_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32161_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32161_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
**** FOUND 10:16:44.34 +18:22:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32162_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32162_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32222_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32222_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32321_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
Preparing report for the candidate 32321_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
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Considering the candidate 32322_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32322_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
**** FOUND 10:57:36.26 +15:44:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32334_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32334_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32356_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
Preparing report for the candidate 32356_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
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Considering the candidate 32372_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32372_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32436_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
Preparing report for the candidate 32436_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
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Considering the candidate 32445_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32445_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
**** FOUND 11:08:39.21 +17:13:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32474_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32474_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32557_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
Preparing report for the candidate 32557_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
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Considering the candidate 32569_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32569_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32622_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32622_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
**** FOUND 10:16:27.39 +16:52:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32624_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32624_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32632_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32632_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
**** FOUND 10:29:40.50 +16:59:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32688_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32688_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32727_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
Preparing report for the candidate 32727_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
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Considering the candidate 32755_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32755_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32786_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32786_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32880_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32880_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
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Considering the candidate 32961_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075
The candidate 32961_fd_Leo-05-Q1b1x1_2026-06-13_23-30-32_20.00sec_-0.00C_LIGHTs_0075 did not pass the final checks
