This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA
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 17.1800 2461208.6800 12.11 11:01:22.11 +21:47:03.6
218.95047 64.44348 galactic Leo Second-epoch detections are separated by 0.5" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.511 Davida -0 -0 1 12.4 -0 0
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:01:22.11 +21:47:03.6: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:01:22.11 +21:47:03.6: 16.11 +/- 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 17.1800* 11 01 22.11 +21 47 03.6 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,2461208.6800,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260617.1800 12.11CV 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 17.1800 2461208.6800 14.75 10:53:18.71 +25:55:44.5
208.75835 63.61097 galactic LMi Second-epoch detections are separated by 8.5" and 11.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:53:18.71 +25:55:44.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:53:18.71 +25:55:44.5: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:53:18.71 +25:55:44.5: 16.17 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461208.6800,14.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260617.1800 14.75CV 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 17.1800 2461208.6800 14.29 11:21:24.84 +19:35:06.5
228.21642 68.04627 galactic Leo Second-epoch detections are separated by 5.3" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:21:24.84 +19:35:06.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:21:24.84 +19:35:06.5: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:21:24.84 +19:35:06.5: 16.13 +/- 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 17.1800* 11 21 24.84 +19 35 06.5 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461208.6800,14.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260617.1800 14.29CV 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 17.1800 2461208.6800 14.53 11:16:20.34 +18:45:06.4
228.87252 66.60865 galactic Leo Second-epoch detections are separated by 7.3" and 11.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:16:20.34 +18:45:06.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:16:20.34 +18:45:06.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:16:20.34 +18:45:06.4: 16.11 +/- 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 17.1800* 11 16 20.34 +18 45 06.4 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
target,2461208.6800,14.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260617.1800 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
Mean magnitude and position on the discovery images:
2026 06 17.1800 2461208.6800 14.98 10:46:56.71 +25:42:41.2
208.70596 62.16199 galactic LMi Second-epoch detections are separated by 6.5" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:46:56.71 +25:42:41.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:56.71 +25:42:41.2: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:56.71 +25:42:41.2: 16.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461208.6800,14.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260617.1800 14.98CV 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 17.1800 2461208.6800 14.99 10:51:40.02 +17:43:35.4
225.42982 60.85805 galactic Leo Second-epoch detections are separated by 8.6" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:51:40.02 +17:43:35.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:40.02 +17:43:35.4: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:40.02 +17:43:35.4: 16.06 +/- 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 17.1800* 10 51 40.02 +17 43 35.4 15.0 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
target,2461208.6800,14.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260617.1800 14.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
First image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Last image: 2461208.68021581 17.06.2026 04:19:20.646 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 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): 4540
Objects passed selection criteria: 4527
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 4001
Average stars matched: 3911 (97.7506 %)
Memory usage VmPeak: 111020 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 16 23:49:28 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
First image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Last image: 2461208.68021581 17.06.2026 04:19:20.646 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 102
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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: 15 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): 23968
Objects passed selection criteria: 23901
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 26192.8
Average stars matched: 21243.2 (81.1035 %)
Memory usage VmPeak: 132288 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 16 23:51:23 CDT 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR_OR_FILE= /var/www/nmw_calibration/TTUQ2b1x1/darks
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 15.0
FLAT_FIELD_DIR_OR_FILE= /var/www/nmw_calibration/TTUQ2b1x1/flats
FRAME_EDGE_OFFSET_PIX= 600
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= V36
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 8000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 4000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 4
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Leo-03-Q2b1x1
#######################################
########### Starting Leo-03-Q2b1x1 ###########
Processing Leo-03-Q2b1x1
WARNING: server tau is low on disk space, only 96999 MB free at /data_ssd/NMW-TexasTech/workdir
WARNING: server tau is low on disk space, only 96999 MB free at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.png' -> 'transient_report/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits_preview.png'
Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
renamed 'Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.png' -> 'transient_report/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits_preview.png'
Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 477.6453
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 450.1253
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1101.4689
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 432.1983
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1103.2106
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 431.3667
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.30604
INFO: SECOND_EPOCH__SD_ratio= 0.002
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR_OR_FILE=/var/www/nmw_calibration/TTUQ2b1x1/darks FLAT_FIELD_DIR_OR_FILE=/var/www/nmw_calibration/TTUQ2b1x1/flats
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= 10.0 / [degC] CCD temperature setpoint
CCD-TEMP= 9.9 / [degC] CCD temperature
FOCTEMP = 27.3500003814697 / [degC] Focuser temperature
AMBTEMP = 27.6 / [degC] Ambient air temperature
No matching dark image found
try_to_calibrate_the_input_frame(): cannot find a good dark frame by running util/find_best_dark.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= 10.0 / [degC] CCD temperature setpoint
CCD-TEMP= 9.9 / [degC] CCD temperature
FOCTEMP = 27.3400001525879 / [degC] Focuser temperature
AMBTEMP = 27.7 / [degC] Ambient air temperature
No matching dark image found
try_to_calibrate_the_input_frame(): cannot find a good dark frame by running util/find_best_dark.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.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: 2461208.67970130
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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits exists and is non-empty
Saving wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits exists and is non-empty
Saving wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits'
wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits exists and is non-empty
Saving wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits'
wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits exists and is non-empty
Saving wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (1st reference image)
verification OK: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:04:39.947 +21:57:23.32 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits (1st new image)
verification OK: wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
Image size: 937.3'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:04:37.514 +22:00:26.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:04:37.514 +22:00:26.98
Angular distance between the image centers 0.0519 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits (2nd new image)
verification OK: wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
Image size: 937.3'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:04:34.415 +22:01:07.50 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:04:34.415 +22:01:07.50
Angular distance between the image centers 0.0658 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:04:37.514 +22:00:26.98
Second-epoch second image center 11:04:34.415 +22:01:07.50
Angular distance between the image centers 0.01643 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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits &> /tmp/tmp.wvtFLpgGRd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits &> /tmp/tmp.Mnb2NFHUm2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits &> /tmp/tmp.QlrskOXZJ0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits &> /tmp/tmp.3dBoNqgOma
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
The reference image (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits) and catalog (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat) found
'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat' -> 'wcsmag.cat'
Read 5863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6102 to 175.2048 deg, Dec +16.0221 to +27.5014 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 157.6102 to 175.2048 deg, Dec 16.0221 to 27.5014 deg
Loaded 4338 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): 3191 out of 3323 total matches.
Matched with Tycho-2 3323 out of 5863 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.852600
a=0.000000 b=1.000000 c=22.852600
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6102 to 175.2048 deg, Dec +16.0221 to +27.5014 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 157.6102 to 175.2048 deg, Dec 16.0221 to 27.5014 deg
Loaded 4338 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): 3191 out of 3323 total matches.
Matched with Tycho-2 3323 out of 5863 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (aperture=6.1)
Read 5873 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6053 to 175.1804 deg, Dec +16.0221 to +27.5014 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 157.6053 to 175.1804 deg, Dec 16.0221 to 27.5014 deg
Loaded 4338 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): 3172 out of 3318 total matches.
Matched with Tycho-2 3318 out of 5873 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.1 pix Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
2.3 pix Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
2.3 pix Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
2.1 pix wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.1 pix wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Limiting magnitude estimates:
15.4 mag. Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
15.4 mag. Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
15.0 mag. Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
15.0 mag. Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wvtFLpgGRd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=376, passed=5863
Got 5863 stars (including 5481 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
util/solve_plate_with_UCAC5 got 5863 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits N_match=944 sigma_overall_arcsec=0.274 sigma_q1_arcsec=0.217 sigma_q2_arcsec=0.328 sigma_q3_arcsec=0.235 sigma_q4_arcsec=0.295 n_q1=218 n_q2=240 n_q3=245 n_q4=241 worst_quadrant_to_overall_ratio=1.199
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Mnb2NFHUm2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=393, passed=5873
Got 5873 stars (including 5475 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat
util/solve_plate_with_UCAC5 got 5873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits N_match=943 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.277 sigma_q2_arcsec=0.404 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.301 n_q1=217 n_q2=238 n_q3=247 n_q4=241 worst_quadrant_to_overall_ratio=1.306
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QlrskOXZJ0 (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_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.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_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=292, passed=4352
Got 4352 stars (including 4059 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat
util/solve_plate_with_UCAC5 got 4352 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.2)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 4271 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.2)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 4272 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 4272 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 940 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits N_match=940 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.297 sigma_q2_arcsec=0.399 sigma_q3_arcsec=0.334 sigma_q4_arcsec=0.376 n_q1=225 n_q2=258 n_q3=206 n_q4=251 worst_quadrant_to_overall_ratio=1.111
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits -region wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.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.3dBoNqgOma (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_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.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_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=302, passed=4344
Got 4344 stars (including 4041 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat
util/solve_plate_with_UCAC5 got 4344 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 4262 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 533 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 4259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 4259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits N_match=942 sigma_overall_arcsec=0.365 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.427 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.365 n_q1=231 n_q2=261 n_q3=202 n_q4=248 worst_quadrant_to_overall_ratio=1.171
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits -region wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits sigma_overall=0.274 worst_q_ratio=1.199
ref2=Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits sigma_overall=0.310 worst_q_ratio=1.306
new1=Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits sigma_overall=0.359 worst_q_ratio=1.111
new2=Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits sigma_overall=0.365 worst_q_ratio=1.171
reference average sigma_overall=0.292 worst_q_ratio=1.2525
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176_astrometric_residuals.png (944 matched stars from wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177_astrometric_residuals.png (943 matched stars from wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104_astrometric_residuals.png (940 matched stars from wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105_astrometric_residuals.png (942 matched stars from wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits'
Saving fully-calibrated image wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits'
Preparing the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:05:05.45 +23:05:11.2: 12.41 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:58:10.39 +23:13:10.7: 12.54 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:01:11.80 +22:39:09.8: 12.51 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:02:17.96 +22:48:43.2: 12.33 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:01:43.77 +23:31:53.5: 12.45 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:01:22.11 +21:47:03.6: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:59:05.49 +24:15:11.7: 12.55 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:07:18.10 +20:57:54.5: 12.43 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:57:23.67 +22:44:42.3: 12.58 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:53:35.14 +22:25:36.4: 12.54 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:05:05.45 +23:05:11.2: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter REJECTED candidate at 11:05:05.45 +23:05:11.2: ref_mag=12.42 +/- 0.01 new_mean_mag=12.2271 delta=0.19 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:07:18.10 +20:57:54.5: 12.46 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:58:10.39 +23:13:10.7: 12.51 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:01:11.80 +22:39:09.8: 12.55 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:59:05.49 +24:15:11.7: 12.60 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:02:17.96 +22:48:43.2: 12.33 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:01:22.11 +21:47:03.6: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:57:23.67 +22:44:42.3: 12.61 +/- 0.01 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:01:43.77 +23:31:53.5: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 11:07:18.10 +20:57:54.5: ref_mag=12.45 +/- 0.01 new_mean_mag=12.2105 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter REJECTED candidate at 10:58:10.39 +23:13:10.7: ref_mag=12.53 +/- 0.01 new_mean_mag=12.2946 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:01:11.80 +22:39:09.8: ref_mag=12.53 +/- 0.01 new_mean_mag=12.3149 delta=0.21 (need > 0.90)
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter REJECTED candidate at 11:02:17.96 +22:48:43.2: ref_mag=12.33 +/- 0.01 new_mean_mag=12.1733 delta=0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:57:23.67 +22:44:42.3: ref_mag=12.59 +/- 0.01 new_mean_mag=12.3628 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:59:05.49 +24:15:11.7: ref_mag=12.57 +/- 0.01 new_mean_mag=12.3998 delta=0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:01:43.77 +23:31:53.5: ref_mag=12.46 +/- 0.01 new_mean_mag=12.2823 delta=0.18 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:53:35.14 +22:25:36.4: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter REJECTED candidate at 10:53:35.14 +22:25:36.4: ref_mag=12.55 +/- 0.01 new_mean_mag=12.3736 delta=0.18 (need > 0.90)
Adding exclusion_list_local.txt__out20277.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20238_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 20238_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
**** FOUND 10:56:23.21 +22:21:28.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20277_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
Preparing report for the candidate 20277_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
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Considering the candidate 20285_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 20285_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20294_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 20294_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20295_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 20295_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 20299_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 20299_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 20300_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 20300_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 20305_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 20305_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20306_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 20306_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20310_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 20310_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20312_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 20312_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:01:22.11 +21:47:03.6
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits exists and is non-empty
wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits exists and is non-empty
wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits exists and is non-empty
wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (1st reference image)
verification OK: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:04:39.947 +21:57:23.32 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits (1st new image)
verification OK: wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
Image size: 937.3'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:04:37.514 +22:00:26.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:04:37.514 +22:00:26.98
Angular distance between the image centers 0.0519 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits (2nd new image)
verification OK: wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
Image size: 937.3'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:04:34.415 +22:01:07.50 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:04:34.415 +22:01:07.50
Angular distance between the image centers 0.0658 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:04:37.514 +22:00:26.98
Second-epoch second image center 11:04:34.415 +22:01:07.50
Angular distance between the image centers 0.01643 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-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits &> /tmp/tmp.5MonBGujzP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits &> /tmp/tmp.ZqII2drJH1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits &> /tmp/tmp.aeCfQl19AD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits &> /tmp/tmp.WkYWOmxQBs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
Found non-empty wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
The reference image (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits) and catalog (wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat) found
'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat' -> 'wcsmag.cat'
Read 31701 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6097 to 175.2801 deg, Dec +16.0221 to +27.5078 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 157.6097 to 175.2801 deg, Dec 16.0221 to 27.5078 deg
Loaded 4353 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): 3103 out of 3360 total matches.
Matched with Tycho-2 3360 out of 31701 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.749800
a=0.000000 b=1.000000 c=22.749800
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31701 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6097 to 175.2801 deg, Dec +16.0221 to +27.5078 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 157.6097 to 175.2801 deg, Dec 16.0221 to 27.5078 deg
Loaded 4353 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): 3103 out of 3360 total matches.
Matched with Tycho-2 3360 out of 31701 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (aperture=4.8)
Read 31604 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.5943 to 175.2797 deg, Dec +16.0221 to +27.5110 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 157.5943 to 175.2797 deg, Dec 16.0221 to 27.5110 deg
Loaded 4362 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): 3082 out of 3366 total matches.
Matched with Tycho-2 3366 out of 31604 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -> calib.txt_param_ref_wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.0 pix Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
2.4 pix Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
2.4 pix Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
2.0 pix wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.0 pix wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Limiting magnitude estimates:
15.6 mag. Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
15.6 mag. Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
15.2 mag. Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
15.2 mag. Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5MonBGujzP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1119, passed=31691
Got 31691 stars (including 30518 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat
util/solve_plate_with_UCAC5 got 31691 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 31378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 31379 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 31379 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits N_match=943 sigma_overall_arcsec=0.262 sigma_q1_arcsec=0.216 sigma_q2_arcsec=0.305 sigma_q3_arcsec=0.223 sigma_q4_arcsec=0.282 n_q1=220 n_q2=244 n_q3=242 n_q4=237 worst_quadrant_to_overall_ratio=1.165
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ZqII2drJH1 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1160, passed=31589
Got 31589 stars (including 30375 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat
util/solve_plate_with_UCAC5 got 31589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31160 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits N_match=944 sigma_overall_arcsec=0.308 sigma_q1_arcsec=0.276 sigma_q2_arcsec=0.374 sigma_q3_arcsec=0.255 sigma_q4_arcsec=0.308 n_q1=219 n_q2=243 n_q3=244 n_q4=238 worst_quadrant_to_overall_ratio=1.215
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -region wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.aeCfQl19AD (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_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.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_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1139, passed=34174
Got 34174 stars (including 32954 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat
util/solve_plate_with_UCAC5 got 34174 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 907 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 32836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 907 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 32836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 32836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 907 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits N_match=907 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.290 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.349 sigma_q4_arcsec=0.358 n_q1=230 n_q2=237 n_q3=204 n_q4=236 worst_quadrant_to_overall_ratio=1.111
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits -region wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.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.WkYWOmxQBs (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_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.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_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat corresponding to the image wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1296, passed=34289
Got 34289 stars (including 32901 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat
util/solve_plate_with_UCAC5 got 34289 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 904 matched stars entering correct_measured_positions(), 883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 904 matched stars entering correct_measured_positions(), 32899 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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 32898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 32898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 903 stars left (next iteration limit 994)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits N_match=903 sigma_overall_arcsec=0.357 sigma_q1_arcsec=0.312 sigma_q2_arcsec=0.406 sigma_q3_arcsec=0.316 sigma_q4_arcsec=0.372 n_q1=234 n_q2=241 n_q3=196 n_q4=232 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits -region wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.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_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.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_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/wcs_Leo-03-Q2b1x1_2026-06-16_23-18-36_20.00sec_9.90C_LIGHT_0104.fits
Saving fully-calibrated image wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.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_2026-06-16_CI_Leo-03-Q2b1x1_233310_TTUQ2b1x1_2159496_bV8xm2VA/wcs_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105.fits
Preparing the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:16:38.72 +20:01:46.9: 15.09 +/- 0.13 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:05:43.08 +19:03:13.8: 15.22 +/- 0.14 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:57:10.68 +24:51:23.7: 14.55 +/- 0.08 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:14:19.99 +19:36:16.8: 14.77 +/- 0.10 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:32:42.90 +25:30:02.2: 14.53 +/- 0.10 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:58:47.76 +25:09:24.1: 14.87 +/- 0.11 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:06:54.48 +19:14:00.6: 14.88 +/- 0.11 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:08:55.55 +25:53:32.3: 14.52 +/- 0.08 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:23:47.97 +22:30:19.7: 14.49 +/- 0.08 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:31:38.52 +24:08:44.0: 13.97 +/- 0.05 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:16:38.72 +20:01:46.9: 14.79 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.08
Forced photometry filter REJECTED candidate at 11:16:38.72 +20:01:46.9: ref_mag=14.91 +/- 0.08 new_mean_mag=14.5833 delta=0.32 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:57:10.68 +24:51:23.7: 14.58 +/- 0.08 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:05:43.08 +19:03:13.8: 15.03 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.06
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:14:19.99 +19:36:16.8: 14.67 +/- 0.09 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:08:55.55 +25:53:32.3: 14.57 +/- 0.08 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:58:47.76 +25:09:24.1: 14.89 +/- 0.11 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:32:42.90 +25:30:02.2: 14.35 +/- 0.08 detection
Forced photometry filter REJECTED candidate at 10:57:10.68 +24:51:23.7: ref_mag=14.57 +/- 0.06 new_mean_mag=14.7922 delta=-0.22 (need > 0.90)
Forced photometry reference-image weighted average: 15.11 +/- 0.09
Forced photometry filter REJECTED candidate at 11:05:43.08 +19:03:13.8: ref_mag=15.11 +/- 0.09 new_mean_mag=14.7485 delta=0.36 (need > 0.90)
Forced photometry reference-image weighted average: 14.72 +/- 0.07
Forced photometry reference-image weighted average: 14.54 +/- 0.06
Forced photometry reference-image weighted average: 14.88 +/- 0.08
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:06:54.48 +19:14:00.6: 15.26 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.06
Forced photometry filter REJECTED candidate at 11:14:19.99 +19:36:16.8: ref_mag=14.72 +/- 0.07 new_mean_mag=14.5897 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:08:55.55 +25:53:32.3: ref_mag=14.54 +/- 0.06 new_mean_mag=14.4662 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:58:47.76 +25:09:24.1: ref_mag=14.88 +/- 0.08 new_mean_mag=14.7592 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:32:42.90 +25:30:02.2: ref_mag=14.42 +/- 0.06 new_mean_mag=14.5849 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 15.01 +/- 0.09
Forced photometry filter REJECTED candidate at 11:06:54.48 +19:14:00.6: ref_mag=15.01 +/- 0.09 new_mean_mag=14.7773 delta=0.23 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:23:47.97 +22:30:19.7: 14.46 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.06
Forced photometry filter REJECTED candidate at 11:23:47.97 +22:30:19.7: ref_mag=14.48 +/- 0.06 new_mean_mag=14.2054 delta=0.27 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:31:38.52 +24:08:44.0: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter REJECTED candidate at 11:31:38.52 +24:08:44.0: ref_mag=13.93 +/- 0.04 new_mean_mag=14.0493 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:11:39.51 +25:05:24.9: 14.41 +/- 0.07 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:01:55.36 +24:40:49.6: 14.05 +/- 0.05 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:07:13.70 +21:00:04.7: 13.05 +/- 0.02 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:09:25.33 +20:09:29.1: 13.65 +/- 0.04 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:33:47.37 +23:24:14.3: 13.12 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:28:37.87 +23:26:13.1: 13.44 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:11:39.51 +25:05:24.9: 14.35 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.05
Forced photometry filter REJECTED candidate at 11:11:39.51 +25:05:24.9: ref_mag=14.38 +/- 0.05 new_mean_mag=14.1639 delta=0.21 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:01:55.36 +24:40:49.6: 14.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.11 +/- 0.04
Forced photometry filter REJECTED candidate at 11:01:55.36 +24:40:49.6: ref_mag=14.11 +/- 0.04 new_mean_mag=13.9560 delta=0.16 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:07:13.70 +21:00:04.7: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.01
Forced photometry filter REJECTED candidate at 11:07:13.70 +21:00:04.7: ref_mag=13.08 +/- 0.01 new_mean_mag=12.8013 delta=0.27 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:09:25.33 +20:09:29.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Forced photometry filter REJECTED candidate at 11:09:25.33 +20:09:29.1: ref_mag=13.65 +/- 0.03 new_mean_mag=13.6220 delta=0.02 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:33:47.37 +23:24:14.3: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter REJECTED candidate at 11:33:47.37 +23:24:14.3: ref_mag=13.11 +/- 0.02 new_mean_mag=13.6951 delta=-0.58 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:28:37.87 +23:26:13.1: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter REJECTED candidate at 11:28:37.87 +23:26:13.1: ref_mag=13.39 +/- 0.02 new_mean_mag=13.7533 delta=-0.37 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:53:18.71 +25:55:44.5: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:29:33.91 +18:14:01.6: 13.91 +/- 0.05 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:21:24.84 +19:35:06.5: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:16:20.34 +18:45:06.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:53:18.71 +25:55:44.5: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:21:24.84 +19:35:06.5: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:29:33.91 +18:14:01.6: 13.89 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Forced photometry filter REJECTED candidate at 11:29:33.91 +18:14:01.6: ref_mag=13.90 +/- 0.04 new_mean_mag=14.1691 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:16:53.28 +18:15:48.6: 15.02 +/- 0.15 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:46:56.71 +25:42:41.2: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:09:36.51 +23:52:51.4: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:16:20.34 +18:45:06.4: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:08:24.08 +22:41:30.9: 14.97 +/- 0.12 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:16:53.28 +18:15:48.6: 14.92 +/- 0.13 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:46:56.71 +25:42:41.2: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:09:36.51 +23:52:51.4: 16.23 +/- 0.36 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.09
Forced photometry reference-image weighted average: 16.23 +/- 0.36
Forced photometry filter REJECTED candidate at 11:16:53.28 +18:15:48.6: ref_mag=14.96 +/- 0.09 new_mean_mag=14.6858 delta=0.28 (need > 0.90)
Forced photometry filter KEPT candidate at 11:09:36.51 +23:52:51.4: ref_mag=16.23 +/- 0.36 new_mean_mag=14.6568 delta=1.57 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:14:15.12 +21:45:21.9: 15.35 +/- 0.16 detection
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:08:24.08 +22:41:30.9: 14.91 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.08
Forced photometry filter REJECTED candidate at 11:08:24.08 +22:41:30.9: ref_mag=14.94 +/- 0.08 new_mean_mag=14.7839 delta=0.15 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:51:40.02 +17:43:35.4: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:14:15.12 +21:45:21.9: 15.40 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.38 +/- 0.12
Forced photometry filter REJECTED candidate at 11:14:15.12 +21:45:21.9: ref_mag=15.38 +/- 0.12 new_mean_mag=14.8045 delta=0.57 (need > 0.90)
Forced photometry on wcs_Leo-03-Q2b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:51:40.02 +17:43:35.4: 16.06 +/- 99.00 upperlimit
Adding exclusion_list_gaiadr2.txt__out57091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out55224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58697.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 51731_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51731_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51735_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51735_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51738_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51738_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51740_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51740_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51745_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51745_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51749_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51749_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51753_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51753_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51757_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51757_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51759_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51759_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 51760_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51760_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:22:38.60 +22:01:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51763_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51763_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51765_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51765_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51766_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51766_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51769_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51769_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51776_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51776_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 51998_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 51998_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
**** FOUND 10:56:23.20 +22:21:28.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52196_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 52196_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:01:22.12 +21:47:03.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52264_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 52264_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:07:34.59 +21:09:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52375_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 52375_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
**** FOUND 10:55:27.52 +24:43:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53241_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 53241_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 53485_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 53485_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 53893_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 53893_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:21:02.55 +23:49:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53991_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 53991_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
**** FOUND 10:46:35.67 +24:40:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54101_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 54101_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:00:33.42 +23:43:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54216_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 54216_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 54273_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 54273_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 54422_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 54422_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 54611_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 54611_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 54813_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 54813_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 54924_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 54924_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 55131_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 55131_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 55224_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
Preparing report for the candidate 55224_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
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Considering the candidate 55489_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 55489_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 55903_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
Preparing report for the candidate 55903_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
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Considering the candidate 56065_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 56065_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 56124_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
Preparing report for the candidate 56124_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
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Considering the candidate 56288_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 56288_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 56406_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 56406_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 56541_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 56541_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 56556_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 56556_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 56802_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 56802_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 56952_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
Preparing report for the candidate 56952_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
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Considering the candidate 57091_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 57091_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
**** FOUND 11:09:36.51 +23:52:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 1.370 3995289496270419968 167.40247315662 +23.88115297024 14.7972 13.4033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57237_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 57237_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 57365_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 57365_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 57657_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 57657_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 57683_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 57683_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 58123_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 58123_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 58310_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 58310_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
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Considering the candidate 58431_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 58431_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 58546_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 58546_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 58653_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 58653_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 58697_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
Preparing report for the candidate 58697_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
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Considering the candidate 59505_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 59505_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 59604_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105
The candidate 59604_Leo-03-Q2b1x1_2026-06-16_23-19-20_20.00sec_9.90C_LIGHT_0105 did not pass the final checks
