This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D
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!
TCP 2026 04 17.3837* 13 47 35.06 -17 38 48.1 10.9 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8837,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3837 10.95CV 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
ASAS J143642-2112.6,2461147.8837,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J143642-2112.6 20260417.3837 12.93CV 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
VARIABLE_NAME,2461147.8837,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3837 12.03CV 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 17.3837* 13 57 40.22 -16 31 21.6 12.3 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8837,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3837 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 17.3837* 14 00 37.76 -14 14 02.4 12.6 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8837,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3837 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
VARIABLE_NAME,2461147.8837,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3837 13.08CV 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 17.3837* 13 53 21.02 -17 33 35.9 13.3 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8837,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3837 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
VARIABLE_NAME,2461147.8837,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3837 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461118.89271508 19.03.2026 09:25:20.583 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
First image: 2461118.89271508 19.03.2026 09:25:20.583 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
Last image: 2461147.88400757 17.04.2026 09:12:48.254 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.96
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6940
Objects passed selection criteria: 6932
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 6054.25
Average stars matched: 5940.25 (98.117 %)
Memory usage VmPeak: 112752 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 04:16:56 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: 2461118.89271508 19.03.2026 09:25:20.583 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
First image: 2461118.89271508 19.03.2026 09:25:20.583 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
Last image: 2461147.88400757 17.04.2026 09:12:48.254 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 71
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 15 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 42664
Objects passed selection criteria: 42586
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 40098.2
Average stars matched: 38586.8 (96.2305 %)
Memory usage VmPeak: 143008 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 04:17:52 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
SExtractor catalog cache: saved Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat to cache
SExtractor catalog cache: saved Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.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/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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: 2461147.88334142
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits exists and is non-empty
Saving wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits to local_wcs_cache/
'wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits' -> 'local_wcs_cache/wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits'
wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits exists and is non-empty
Saving wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits to local_wcs_cache/
'wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits' -> 'local_wcs_cache/wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits'
wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits exists and is non-empty
Saving wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits to local_wcs_cache/
'wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits' -> 'local_wcs_cache/wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits'
wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits exists and is non-empty
Saving wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits to local_wcs_cache/
'wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits' -> 'local_wcs_cache/wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits (1st reference image)
verification OK: wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
Image size: 937.5'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 14:13:35.779 -17:58:05.55 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits (1st new image)
verification OK: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Image size: 941.4'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: 14:13:21.696 -17:58:59.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:13:35.779 -17:58:05.55
Second-epoch image center 14:13:21.696 -17:58:59.47
Angular distance between the image centers 0.0578 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits (2nd new image)
verification OK: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.4'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: 14:13:20.855 -17:59:33.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:13:35.779 -17:58:05.55
Second-epoch image center 14:13:20.855 -17:59:33.39
Angular distance between the image centers 0.0640 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 14:13:21.696 -17:58:59.47
Second-epoch second image center 14:13:20.855 -17:59:33.39
Angular distance between the image centers 0.00999 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/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits &> /tmp/tmp.xHqWUqbdjH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits &> /tmp/tmp.d0vqYIYtn6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits &> /tmp/tmp.NM4EQ2Ptup
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits &> /tmp/tmp.vDwX3fmTLN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.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_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits and wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.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_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits and wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat
Found non-empty wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits and wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat
The reference image (wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits) and catalog (wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat) found
'wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat' -> 'wcsmag.cat'
Read 7257 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 204.8167 to 221.7383 deg, Dec -23.2629 to -12.4395 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 204.8167 to 221.7383 deg, Dec -23.2629 to -12.4395 deg
Loaded 5528 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): 4457 out of 4557 total matches.
Matched with Tycho-2 4557 out of 7257 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854933
a=0.000000 b=1.000000 c=22.854933
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
2.3 pix Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
2.2 pix fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
2.2 pix fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Limiting magnitude estimates:
14.9 mag. Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
14.9 mag. Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
14.5 mag. fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
14.5 mag. fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.6 (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.xHqWUqbdjH (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/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits' -> 'wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
WCS_IMAGE_NAME=wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
WCS-calibrated image found: wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
Checking if the catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat corresponding to the image wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits alredy exist and is non-empty...
Catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat corresponding to the image wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
WCS catalog name: wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=384, passed=7257
Got 7257 stars (including 6865 good ones) from the SExtractor catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat
util/solve_plate_with_UCAC5 got 7257 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7182 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 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits -region wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.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.d0vqYIYtn6 (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/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits' -> 'wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
WCS-calibrated image found: wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
Checking if the catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat corresponding to the image wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat corresponding to the image wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
WCS catalog name: wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=388, passed=7101
Got 7101 stars (including 6700 good ones) from the SExtractor catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat
util/solve_plate_with_UCAC5 got 7101 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7018 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 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits -region wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.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.NM4EQ2Ptup (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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS_IMAGE_NAME=wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS-calibrated image found: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Checking if the catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat corresponding to the image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat corresponding to the image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS catalog name: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=275, passed=5014
Got 5014 stars (including 4733 good ones) from the SExtractor catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
util/solve_plate_with_UCAC5 got 5014 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 4960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 4961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 4961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits -region wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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.vDwX3fmTLN (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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS_IMAGE_NAME=wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS-calibrated image found: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Checking if the catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat corresponding to the image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat corresponding to the image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS catalog name: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=275, passed=4998
Got 4998 stars (including 4713 good ones) from the SExtractor catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat
util/solve_plate_with_UCAC5 got 4998 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits -region wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits'
Saving fully-calibrated image wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits'
Saving fully-calibrated image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits'
Saving fully-calibrated image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits'
Preparing the HTML report for the field Vir-14-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20339.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20277_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 20277_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:25:27.39 -19:57:55.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20339_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
Preparing report for the candidate 20339_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20394_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 20394_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:43:09.34 -17:20:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00462_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 00462_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:28:45.14 -13:28:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00410_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 00410_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:10:21.41 -13:18:15.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03758_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 03758_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:04:52.36 -18:21:53.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Vir-14-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:47:35.06 -17:38:48.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
SExtractor catalog cache: saved Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat to cache
SExtractor catalog cache: saved Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
Creating symlink local_wcs_cache/wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits exists and is non-empty
wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits exists and is non-empty
wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits exists and is non-empty
wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits (1st reference image)
verification OK: wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
Image size: 937.5'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 14:13:35.779 -17:58:05.55 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits (1st new image)
verification OK: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Image size: 941.4'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: 14:13:21.696 -17:58:59.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:13:35.779 -17:58:05.55
Second-epoch image center 14:13:21.696 -17:58:59.47
Angular distance between the image centers 0.0578 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits (2nd new image)
verification OK: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Image size: 941.4'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: 14:13:20.855 -17:59:33.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:13:35.779 -17:58:05.55
Second-epoch image center 14:13:20.855 -17:59:33.39
Angular distance between the image centers 0.0640 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 14:13:21.696 -17:58:59.47
Second-epoch second image center 14:13:20.855 -17:59:33.39
Angular distance between the image centers 0.00999 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/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits &> /tmp/tmp.xGrUvZ32qm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits &> /tmp/tmp.mfWJysN0Cy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits &> /tmp/tmp.tEgwofQOMm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits &> /tmp/tmp.GzI9wfNStz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.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_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits and wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.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_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits and wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat
Found non-empty wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits and wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat
The reference image (wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits) and catalog (wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat) found
'wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat' -> 'wcsmag.cat'
Read 43328 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 204.7760 to 221.7410 deg, Dec -23.2765 to -12.4172 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 204.7760 to 221.7410 deg, Dec -23.2765 to -12.4172 deg
Loaded 5554 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): 4389 out of 4738 total matches.
Matched with Tycho-2 4738 out of 43328 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.728059
a=0.000000 b=1.000000 c=22.728059
From vast_summary.log: estimated ref. image limiting mag.: -7.72
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 65 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
2.2 pix Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
2.0 pix fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
2.0 pix fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Limiting magnitude estimates:
15.0 mag. Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
15.0 mag. Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
14.7 mag. fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
14.7 mag. fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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.xGrUvZ32qm (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/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits' -> 'wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
WCS_IMAGE_NAME=wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
WCS-calibrated image found: wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
Checking if the catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat corresponding to the image wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits alredy exist and is non-empty...
Catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat corresponding to the image wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
WCS catalog name: wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1738, passed=43316
Got 43316 stars (including 41512 good ones) from the SExtractor catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat
util/solve_plate_with_UCAC5 got 43316 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 43025 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 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 43022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 43022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits -region wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.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.mfWJysN0Cy (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/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits' -> 'wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
WCS-calibrated image found: wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
Checking if the catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat corresponding to the image wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat corresponding to the image wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
WCS catalog name: wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1815, passed=44689
Got 44689 stars (including 42810 good ones) from the SExtractor catalog wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat
util/solve_plate_with_UCAC5 got 44689 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 44369 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 44372 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 44371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits -region wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.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.tEgwofQOMm (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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS_IMAGE_NAME=wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS-calibrated image found: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Checking if the catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat corresponding to the image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat corresponding to the image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS catalog name: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1188, passed=36842
Got 36842 stars (including 35599 good ones) from the SExtractor catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
util/solve_plate_with_UCAC5 got 36842 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 36562 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 36564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 36564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits -region wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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.GzI9wfNStz (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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS_IMAGE_NAME=wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS-calibrated image found: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Checking if the catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat corresponding to the image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat corresponding to the image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS catalog name: wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1195, passed=36729
Got 36729 stars (including 35480 good ones) from the SExtractor catalog wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat
util/solve_plate_with_UCAC5 got 36729 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 36416 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 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 36417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 36417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits -region wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/wcs_Vir-14-Q1b1x1_2026-03-19_04-25-20_20.00sec_-14.90C_LIGHT_0146.fits
Saving fully-calibrated image wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/wcs_Vir-14-Q1b1x1_2026-03-19_04-26-07_20.00sec_-14.90C_LIGHT_0147.fits
Saving fully-calibrated image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Saving fully-calibrated image wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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_2026-04-17_CI_Vir-14-Q1b1x1_041352_TTUQ1b1x1_745158_QFqALO6D/wcs_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Preparing the HTML report for the field Vir-14-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out54242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55182.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out54270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55057.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 54242_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54242_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:43:25.31 -16:34:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.819 6295318494154914432 205.85523011111 -16.57165946730 14.1488 13.5193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54243_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54243_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:16:07.15 -14:50:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54248_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54248_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:21:55.55 -15:15:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 0.550 6299450317117387648 215.48130476945 -15.25170340798 14.3022 13.6035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54249_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54249_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:42:36.08 -14:55:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54253_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54253_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:42:27.47 -14:39:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 0.876 6310800579947144192 220.61463108154 -14.66562132557 13.7556 13.1511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54255_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54255_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:05:59.30 -16:55:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 0.830 6297522602651987712 211.49686658429 -16.93137879000 14.1482 13.4948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54258_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54258_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:37:20.73 -15:30:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.950 6286892043198358144 219.33667757603 -15.50584532390 14.0165 13.4568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54259_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54259_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:36:00.45 -19:58:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.094 6280227731423968640 219.00164189586 -19.97692837915 13.4993 12.7631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54262_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54262_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:09:44.15 -15:17:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54266_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54266_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:44:06.49 -22:14:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54270_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
Preparing report for the candidate 54270_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
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Considering the candidate 54274_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54274_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:25:27.69 -19:57:57.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54292_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54292_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:40:18.39 -18:56:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54336_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54336_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:47:35.05 -17:38:48.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54448_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
Preparing report for the candidate 54448_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
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Considering the candidate 54473_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54473_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:04:24.85 -21:45:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54491_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54491_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:25:42.42 -21:24:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54502_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
Preparing report for the candidate 54502_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
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Considering the candidate 54546_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54546_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:50:39.35 -19:52:53.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54551_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54551_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:21:50.81 -19:25:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.977 6283885974111961088 215.46124150473 -19.41981055005 12.8115 12.1153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54552_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54552_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:15:16.83 -18:11:27.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54556_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
Preparing report for the candidate 54556_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
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Considering the candidate 54580_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54580_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:38:29.02 -16:52:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54591_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54591_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:19:08.78 -14:23:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54642_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
Preparing report for the candidate 54642_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
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Considering the candidate 54643_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54643_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:33:41.80 -21:23:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54666_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54666_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:03:18.11 -15:23:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.644 6300979226691400192 210.82550741678 -15.38856536260 13.3405 12.7677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54704_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54704_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:36:43.62 -16:25:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54711_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54711_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:07:55.43 -22:10:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54764_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54764_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:37:40.94 -20:05:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.379 6280187633609336704 219.42022757315 -20.09920904181 13.4016 12.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54792_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
Preparing report for the candidate 54792_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
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Considering the candidate 54831_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54831_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:18:04.06 -14:44:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54870_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54870_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:44:18.98 -12:57:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54891_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54891_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:33:23.00 -19:55:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.621 6283152741591356928 218.34660200848 -19.91705927248 13.8133 13.2734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54946_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54946_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:04:34.56 -17:08:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 3.001 6297515588970329472 211.14338590187 -17.13703661611 13.9401 13.2942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54966_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 54966_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:52:13.15 -15:53:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55030_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55030_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:43:20.34 -14:11:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55057_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
Preparing report for the candidate 55057_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
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Considering the candidate 55153_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55153_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:41:59.15 -17:46:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55180_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55180_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:40:54.58 -22:58:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.068 6278279843496518656 220.22712915192 -22.96741181678 14.0186 13.2519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55182_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55182_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:31:30.14 -23:04:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.349 6279162098498140672 217.87531921128 -23.07197956696 13.9808 13.3361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55188_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55188_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:37:07.60 -21:49:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.837 6279713091262609280 219.28122877839 -21.82138596153 14.2118 13.6422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55202_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55202_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:47:07.06 -12:32:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55205_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55205_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:44:35.30 -22:07:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.705 6288486335058595200 206.14725176001 -22.13078489473 14.1360 13.7580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55225_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55225_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:42:47.15 -13:56:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55240_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55240_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:31:31.36 -20:54:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 1.442 6279702852060859392 217.88043554667 -20.91207941672 14.2714 13.6919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55245_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55245_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:42:14.81 -18:23:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55248_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55248_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:47:24.45 -12:59:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55250_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55250_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:42:35.50 -15:35:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55252_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55252_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:50:37.29 -12:32:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55254_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55254_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:42:57.67 -13:31:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55262_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55262_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:22:21.88 -15:05:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.541 6299460010859600512 215.59101565171 -15.08993533331 14.1536 13.2766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55269_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55269_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:42:43.25 -15:19:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 0.948 6310693961678870016 220.67996044740 -15.31663970545 14.5603 13.9970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55280_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55280_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:46:22.77 -12:53:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55287_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55287_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:33:30.50 -19:43:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.834 6283296124779467904 218.37731893481 -19.72840523149 14.4889 13.9418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55291_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55291_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:44:40.24 -13:40:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55298_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55298_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:07:24.14 -15:24:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.493 6300794577457466368 211.85060771308 -15.41002527514 14.6976 14.1606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55299_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55299_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:48:25.62 -13:24:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 0.796 3612242116422246912 207.10669297767 -13.41640855294 14.5584 13.6697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55319_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55319_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:42:38.76 -14:15:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55330_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55330_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:44:26.47 -12:41:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55360_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55360_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:48:19.69 -12:36:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55367_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 55367_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 13:44:21.51 -13:49:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01987_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 01987_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:10:21.41 -13:18:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02455_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 02455_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 14:28:45.13 -13:28:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23008_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262
The candidate 23008_fd_Vir-14-Q1b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262 did not pass the final checks
