This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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,2461153.8704,12.69,0.05,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 20260423.3704 12.69CV 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
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
ATO J162.8413+33.8665,2461153.8704,12.39,0.05,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
ATO J162.8413+33.8665 20260423.3704 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461153.8704,12.53,0.05,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 20260423.3704 12.53CV 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
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,2461153.8704,12.44,0.05,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 20260423.3704 12.44CV 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
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 04 23.3704* 11 17 09.66 +27 16 31.0 11.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461153.8704,11.93,0.05,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 20260423.3704 11.93CV 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
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,2461153.8704,12.52,0.05,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 20260423.3704 12.52CV 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
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,2461153.8704,12.57,0.05,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 20260423.3704 12.57CV 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
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,2461153.8704,12.72,0.05,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 20260423.3704 12.72CV 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
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,2461153.8704,12.61,0.05,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 20260423.3704 12.61CV 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
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,2461153.8704,12.71,0.05,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 20260423.3704 12.71CV 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: 2461082.84719906 11.02.2026 08:19:47.999 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
First image: 2461082.84719906 11.02.2026 08:19:47.999 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
Last image: 2461153.87069561 23.04.2026 08:53:38.101 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4133
Objects passed selection criteria: 4109
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 2473.75
Average stars matched: 2318 (93.7039 %)
Memory usage VmPeak: 110624 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 03:59:46 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: 2461082.84719906 11.02.2026 08:19:47.999 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
First image: 2461082.84719906 11.02.2026 08:19:47.999 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
Last image: 2461153.87069561 23.04.2026 08:53:38.101 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
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: 7 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): 23397
Objects passed selection criteria: 23296
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 14819
Average stars matched: 13898.8 (93.7901 %)
Memory usage VmPeak: 128188 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 04:01:05 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/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/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
SExtractor catalog cache: saved LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat to cache
SExtractor catalog cache: saved LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.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/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.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: 2461153.87016944
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_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits exists and is non-empty
Saving wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits to local_wcs_cache/
'wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits' -> 'local_wcs_cache/wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits'
wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits exists and is non-empty
Saving wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits to local_wcs_cache/
'wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits' -> 'local_wcs_cache/wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits'
wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits exists and is non-empty
Saving wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits to local_wcs_cache/
'wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits' -> 'local_wcs_cache/wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits'
wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits exists and is non-empty
Saving wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits to local_wcs_cache/
'wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits' -> 'local_wcs_cache/wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits (1st reference image)
verification OK: wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:59:59.831 +30:00:07.37 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits (1st new image)
verification OK: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:00:05.212 +29:59:51.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:59:59.831 +30:00:07.37
Second-epoch image center 11:00:05.212 +29:59:51.73
Angular distance between the image centers 0.0199 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits (2nd new image)
verification OK: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
Image size: 937.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:00:05.889 +30:00:15.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:59:59.831 +30:00:07.37
Second-epoch image center 11:00:05.889 +30:00:15.98
Angular distance between the image centers 0.0220 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 11:00:05.212 +29:59:51.73
Second-epoch second image center 11:00:05.889 +30:00:15.98
Angular distance between the image centers 0.00717 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/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits &> /tmp/tmp.OSr2jomubN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits &> /tmp/tmp.XQCauuawst
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits &> /tmp/tmp.1QFvMIbOzu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits &> /tmp/tmp.ZiKKk29Ezv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
Calibrating the magnitude scale
Found non-empty wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.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_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits and wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat
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_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits and wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat
Found non-empty wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits and wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat
The reference image (wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits) and catalog (wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat) found
'wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat' -> 'wcsmag.cat'
Read 5336 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.3267 to 174.2153 deg, Dec +24.1797 to +35.3396 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 155.3267 to 174.2153 deg, Dec 24.1797 to 35.3396 deg
Loaded 4190 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): 3034 out of 3153 total matches.
Matched with Tycho-2 3153 out of 5336 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.807264
a=0.000000 b=1.000000 c=22.807264
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5336 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.3267 to 174.2153 deg, Dec +24.1797 to +35.3396 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 155.3267 to 174.2153 deg, Dec 24.1797 to 35.3396 deg
Loaded 4190 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): 3034 out of 3153 total matches.
Matched with Tycho-2 3153 out of 5336 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits via Tycho-2
Forced-photometry filter: calibrated wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits -> calib.txt_param_ref_wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits (aperture=6.1)
Read 5497 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.2958 to 174.2151 deg, Dec +24.1797 to +35.3396 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 155.2958 to 174.2151 deg, Dec 24.1797 to 35.3396 deg
Loaded 4198 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): 3026 out of 3157 total matches.
Matched with Tycho-2 3157 out of 5497 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits via Tycho-2
Forced-photometry filter: calibrated wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits -> calib.txt_param_ref_wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
2.1 pix LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
2.6 pix fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
2.6 pix fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
2.1 pix wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
2.1 pix wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
Limiting magnitude estimates:
15.3 mag. LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
15.3 mag. LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
12.2 mag. fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
12.6 mag. fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 10.1 (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.OSr2jomubN (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/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits' -> 'wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
WCS_IMAGE_NAME=wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
WCS-calibrated image found: wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
Checking if the catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits alredy exist and is non-empty...
Catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
WCS catalog name: wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=369, passed=5336
Got 5336 stars (including 4961 good ones) from the SExtractor catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat
util/solve_plate_with_UCAC5 got 5336 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 5282 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 5288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 960 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits -region wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.XQCauuawst (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/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits' -> 'wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
WCS_IMAGE_NAME=wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
WCS-calibrated image found: wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
Checking if the catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits alredy exist and is non-empty...
Catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
WCS catalog name: wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=380, passed=5497
Got 5497 stars (including 5109 good ones) from the SExtractor catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat
util/solve_plate_with_UCAC5 got 5497 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 570 to 628 (Dec 24.2 to 35.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits -region wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1QFvMIbOzu (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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
WCS-calibrated image found: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
Checking if the catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
WCS catalog name: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=33, passed=966
Got 966 stars (including 931 good ones) from the SExtractor catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat
util/solve_plate_with_UCAC5 got 966 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 877 matched stars entering correct_measured_positions(), 830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 877 matched stars entering correct_measured_positions(), 907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 879 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 879 stars left (next iteration limit 964)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits -region wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ZiKKk29Ezv (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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
WCS_IMAGE_NAME=wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
WCS-calibrated image found: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
Checking if the catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits alredy exist and is non-empty...
Catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
WCS catalog name: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=42, passed=990
Got 990 stars (including 945 good ones) from the SExtractor catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat
util/solve_plate_with_UCAC5 got 990 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 890 matched stars entering correct_measured_positions(), 863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 890 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 892 stars left (next iteration limit 979)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits -region wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits'
Saving fully-calibrated image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits'
Preparing the HTML report for the field LMi-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field LMi-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
SExtractor catalog cache: saved LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat to cache
SExtractor catalog cache: saved LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
Creating symlink local_wcs_cache/wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
Creating symlink local_wcs_cache/wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
Creating symlink local_wcs_cache/wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.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_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits exists and is non-empty
wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits exists and is non-empty
wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits exists and is non-empty
wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits (1st reference image)
verification OK: wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:59:59.831 +30:00:07.37 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits (1st new image)
verification OK: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
Image size: 937.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:00:05.212 +29:59:51.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:59:59.831 +30:00:07.37
Second-epoch image center 11:00:05.212 +29:59:51.73
Angular distance between the image centers 0.0199 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits (2nd new image)
verification OK: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
Image size: 937.9'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:00:05.889 +30:00:15.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:59:59.831 +30:00:07.37
Second-epoch image center 11:00:05.889 +30:00:15.98
Angular distance between the image centers 0.0220 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 11:00:05.212 +29:59:51.73
Second-epoch second image center 11:00:05.889 +30:00:15.98
Angular distance between the image centers 0.00717 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/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits &> /tmp/tmp.dAS4Y4Gnj8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits &> /tmp/tmp.aBopKXfmj5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits &> /tmp/tmp.NpykGDciYm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits &> /tmp/tmp.1KYEnIzFRv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
Calibrating the magnitude scale
Found non-empty wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.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_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits and wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat
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_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits and wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat
Found non-empty wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits and wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat
The reference image (wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits) and catalog (wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat) found
'wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat' -> 'wcsmag.cat'
Read 29361 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.1981 to 174.3206 deg, Dec +24.1797 to +35.3577 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 155.1981 to 174.3206 deg, Dec 24.1797 to 35.3577 deg
Loaded 4257 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): 2970 out of 3227 total matches.
Matched with Tycho-2 3227 out of 29361 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.689801
a=0.000000 b=1.000000 c=22.689801
From vast_summary.log: estimated ref. image limiting mag.: -7.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29361 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.1981 to 174.3206 deg, Dec +24.1797 to +35.3577 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 155.1981 to 174.3206 deg, Dec 24.1797 to 35.3577 deg
Loaded 4257 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): 2970 out of 3227 total matches.
Matched with Tycho-2 3227 out of 29361 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits via Tycho-2
Forced-photometry filter: calibrated wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits -> calib.txt_param_ref_wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits (aperture=4.8)
Read 29934 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 155.1979 to 174.2948 deg, Dec +24.1797 to +35.3537 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 155.1979 to 174.2948 deg, Dec 24.1797 to 35.3537 deg
Loaded 4251 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): 2969 out of 3228 total matches.
Matched with Tycho-2 3228 out of 29934 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits via Tycho-2
Forced-photometry filter: calibrated wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits -> calib.txt_param_ref_wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
1.9 pix LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
2.2 pix fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
2.3 pix fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
1.9 pix wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
1.9 pix wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
Limiting magnitude estimates:
15.5 mag. LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
15.5 mag. LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
13.0 mag. fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
12.8 mag. fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 12.6 (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.dAS4Y4Gnj8 (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/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits' -> 'wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
WCS_IMAGE_NAME=wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
WCS-calibrated image found: wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
Checking if the catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits alredy exist and is non-empty...
Catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits
WCS catalog name: wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1100, passed=29346
Got 29346 stars (including 28196 good ones) from the SExtractor catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat
util/solve_plate_with_UCAC5 got 29346 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 29100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 29100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 29100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits -region wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-19-47_20.00sec_-15.00C_LIGHT_0366.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.aBopKXfmj5 (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/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits' -> 'wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
WCS_IMAGE_NAME=wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
WCS-calibrated image found: wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
Checking if the catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits alredy exist and is non-empty...
Catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat corresponding to the image wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits
WCS catalog name: wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1153, passed=29920
Got 29920 stars (including 28705 good ones) from the SExtractor catalog wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat
util/solve_plate_with_UCAC5 got 29920 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 29681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 29681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 29681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits -region wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_LMi-02-Q2b1x1_2026-02-11_02-20-49_20.00sec_-14.90C_LIGHT_0367.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NpykGDciYm (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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
WCS-calibrated image found: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
Checking if the catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
WCS catalog name: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=100, passed=6538
Got 6538 stars (including 6424 good ones) from the SExtractor catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat
util/solve_plate_with_UCAC5 got 6538 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits -region wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1KYEnIzFRv (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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
WCS_IMAGE_NAME=wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
WCS-calibrated image found: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
Checking if the catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits alredy exist and is non-empty...
Catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
WCS catalog name: wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=102, passed=6572
Got 6572 stars (including 6458 good ones) from the SExtractor catalog wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat
util/solve_plate_with_UCAC5 got 6572 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 6433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 6433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 6433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 939 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits -region wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-52-52_20.00sec_-5.00C_LIGHT_0230.fits
Saving fully-calibrated image wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.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_2026-04-23_CI_LMi-02-Q2b1x1_035634_TTUQ2b1x1_1300715_x8DB9lXu/wcs_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231.fits
Preparing the HTML report for the field LMi-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out06555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28470.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: 5s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33306_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
The candidate 33306_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29244_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
The candidate 29244_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231 did not pass the final checks
**** FOUND 11:18:09.61 +31:31:28.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22958_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
Preparing report for the candidate 22958_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22691_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
Preparing report for the candidate 22691_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28470_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
Preparing report for the candidate 28470_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24736_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
Preparing report for the candidate 24736_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06555_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
Preparing report for the candidate 06555_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21127_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
Preparing report for the candidate 21127_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25323_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
Preparing report for the candidate 25323_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22283_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
Preparing report for the candidate 22283_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25458_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
Preparing report for the candidate 25458_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24462_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
Preparing report for the candidate 24462_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25158_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231
The candidate 25158_fd_LMi-02-Q2b1x1_2026-04-23_03-53-38_20.00sec_-4.90C_LIGHT_0231 did not pass the final checks
