This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J142845-1329.0,2461139.9802,10.67,0.05,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 J142845-1329.0 20260409.4802 10.67CV 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,2461139.9802,11.61,0.05,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 20260409.4802 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.9802,11.94,0.05,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 20260409.4802 11.94CV 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,2461139.9802,12.37,0.05,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 20260409.4802 12.37CV 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,2461139.9802,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.4802 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 09.4802* 14 14 36.21 -10 16 56.0 13.5 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,2461139.9802,13.51,0.05,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 20260409.4802 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 09.4802* 14 11 26.22 -08 11 26.0 13.5 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,2461139.9802,13.54,0.05,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 20260409.4802 13.54CV 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 09.4802* 14 42 00.59 -05 49 57.2 11.9 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
XY Vir,2461139.9802,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
XY Vir 20260409.4802 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 09.4802* 14 15 44.59 -05 52 09.2 11.4 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
CF Vir,2461139.9802,11.39,0.05,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
CF Vir 20260409.4802 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
First image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Last image: 2461139.98055750 09.04.2026 11:31:50.168 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.20
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: 5 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): 5761
Objects passed selection criteria: 5735
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 4421.25
Average stars matched: 4322.5 (97.7665 %)
Memory usage VmPeak: 111756 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 06:35:01 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: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
First image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Last image: 2461139.98055750 09.04.2026 11:31:50.168 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 78
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.91
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: 12 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): 32057
Objects passed selection criteria: 32015
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 27916.5
Average stars matched: 26746.8 (95.8098 %)
Memory usage VmPeak: 134980 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 06:35:56 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/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
SExtractor catalog cache: saved Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.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: 2461139.97981815
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits exists and is non-empty
Saving wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits to local_wcs_cache/
'wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'local_wcs_cache/wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
Saving wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits to local_wcs_cache/
'wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'local_wcs_cache/wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits'
wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:15.515 -09:59:18.46
Angular distance between the image centers 0.0552 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:14.341 -09:58:49.74
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 14:34:15.515 -09:59:18.46
Second-epoch second image center 14:34:14.341 -09:58:49.74
Angular distance between the image centers 0.00932 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/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits &> /tmp/tmp.7Ua2p4PEGD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.80i1tzHFh1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits &> /tmp/tmp.fO6VF7eZtH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits &> /tmp/tmp.M45elBiBjZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
Found non-empty wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
The reference image (wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits) and catalog (wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat) found
'wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat' -> 'wcsmag.cat'
Read 5992 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.5294 to 226.6314 deg, Dec -15.2867 to -4.6831 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 210.5294 to 226.6314 deg, Dec -15.2867 to -4.6831 deg
Loaded 4504 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): 3597 out of 3683 total matches.
Matched with Tycho-2 3683 out of 5992 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.927740
a=0.000000 b=1.000000 c=22.927740
From vast_summary.log: estimated ref. image limiting mag.: -8.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.73
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.73
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
2.4 pix Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
2.2 pix fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
2.2 pix fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
Limiting magnitude estimates:
14.7 mag. Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
14.8 mag. Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
14.1 mag. fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
14.0 mag. fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.7Ua2p4PEGD (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/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Checking if the catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS catalog name: wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=377, passed=5992
Got 5992 stars (including 5611 good ones) from the SExtractor catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 5992 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
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: 970 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 972 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(), 5898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 971 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_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits -region wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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.80i1tzHFh1 (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/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=404, passed=5931
Got 5931 stars (including 5520 good ones) from the SExtractor catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 5931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 5842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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.fO6VF7eZtH (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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
Checking if the catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
WCS catalog name: wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=407, passed=3088
Got 3088 stars (including 2679 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat
util/solve_plate_with_UCAC5 got 3088 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 371 to 431 (Dec -15.6 to -4.2)
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: 970 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 3044 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
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: 970 matched stars entering correct_measured_positions(), 3043 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 3043 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits -region wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.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.M45elBiBjZ (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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
Checking if the catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
WCS catalog name: wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=421, passed=2929
Got 2929 stars (including 2502 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat
util/solve_plate_with_UCAC5 got 2929 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 2889 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 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 2890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 2890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits -region wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.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_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
Saving fully-calibrated image wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
Saving fully-calibrated image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits'
Saving fully-calibrated image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits'
Preparing the HTML report for the field Lib-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out01128.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 20282_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 20282_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:10:21.43 -13:18:15.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20286_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 20286_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:46:16.76 -11:05:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 0.038 6325601999321593344 221.56982336201 -11.09678189897 10.3783 9.9512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20355_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 20355_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:15:44.55 -05:52:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 1.335 3640834503985725696 213.93539692358 -05.86876222884 10.5939 9.3160 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01128_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
Preparing report for the candidate 01128_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Lib-01-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 ####
14:28:45.15 -13:28:57.4
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/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
SExtractor catalog cache: saved Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Creating symlink local_wcs_cache/wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.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_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits exists and is non-empty
wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits exists and is non-empty
wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:15.515 -09:59:18.46
Angular distance between the image centers 0.0552 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:14.341 -09:58:49.74
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 14:34:15.515 -09:59:18.46
Second-epoch second image center 14:34:14.341 -09:58:49.74
Angular distance between the image centers 0.00932 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/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits &> /tmp/tmp.jmO8wxvzeW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.3sgwqOsOLo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits &> /tmp/tmp.mpgiYxoSSe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits &> /tmp/tmp.1IKSjroQ2m
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
Found non-empty wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
The reference image (wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits) and catalog (wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat) found
'wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat' -> 'wcsmag.cat'
Read 33758 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.4848 to 226.6346 deg, Dec -15.2985 to -4.6504 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 210.4848 to 226.6346 deg, Dec -15.2985 to -4.6504 deg
Loaded 4537 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): 3660 out of 3887 total matches.
Matched with Tycho-2 3887 out of 33758 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.771705
a=0.000000 b=1.000000 c=22.771705
From vast_summary.log: estimated ref. image limiting mag.: -7.91
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.86
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 68 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
2.3 pix Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
2.0 pix fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
2.0 pix fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
Limiting magnitude estimates:
14.9 mag. Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
14.9 mag. Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
14.2 mag. fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
14.1 mag. fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jmO8wxvzeW (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/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Checking if the catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS catalog name: wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1364, passed=33748
Got 33748 stars (including 32348 good ones) from the SExtractor catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 33748 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
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: 967 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 33426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
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: 967 matched stars entering correct_measured_positions(), 33426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 33426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits -region wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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.3sgwqOsOLo (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/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1488, passed=34762
Got 34762 stars (including 33241 good ones) from the SExtractor catalog wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 34762 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
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: 967 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
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: 967 matched stars entering correct_measured_positions(), 34351 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34351 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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.mpgiYxoSSe (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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
Checking if the catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
WCS catalog name: wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=869, passed=22698
Got 22698 stars (including 21789 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat
util/solve_plate_with_UCAC5 got 22698 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 22399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 22399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 22399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits -region wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.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.1IKSjroQ2m (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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
Checking if the catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat corresponding to the image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
WCS catalog name: wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=885, passed=21466
Got 21466 stars (including 20543 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat
util/solve_plate_with_UCAC5 got 21466 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 371 to 431 (Dec -15.6 to -4.2)
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(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 21214 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 371 to 431 (Dec -15.6 to -4.2)
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(), 21213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 21213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits -region wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.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_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/wcs_Lib-01-Q1b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Saving fully-calibrated image wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/wcs_Lib-01-Q1b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Saving fully-calibrated image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-30-46_20.00sec_-5.00C_LIGHTs_0287.fits
Saving fully-calibrated image wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.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_2026-04-09_CI_Lib-01-Q1b1x1_063243_TTUQ1b1x1_13462_nE9DnXTN/wcs_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288.fits
Preparing the HTML report for the field Lib-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out50050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out25642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54173.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 53410_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53410_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:56:14.26 -05:56:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.186 6334116754806083072 224.05852937838 -05.94634367746 13.7343 13.0235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53414_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53414_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:23:20.50 -14:43:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 0.891 6299578345798545792 215.83543123609 -14.71791365144 12.9882 12.4481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53418_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53418_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:56:51.66 -12:42:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.063 6312216338607014400 224.21522066289 -12.71043264892 12.7626 12.3301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53419_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53419_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:31:52.39 -07:00:02.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)
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Considering the candidate 53420_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53420_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:51:32.76 -13:49:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 0.466 6311372978828634752 222.88654635854 -13.82651016745 12.6530 11.9749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53421_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53421_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:56:41.22 -13:58:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53422_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53422_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:38:45.08 -09:23:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.137 6326817505130128384 219.68787808379 -09.39614607114 12.5897 11.8016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53423_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53423_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:41:46.11 -05:16:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.204 6337789188066919424 220.44217796895 -05.27139616385 12.5119 12.0094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53424_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53424_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:57:15.71 -14:08:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.515 6310378848518593536 224.31587613981 -14.13852484847 12.3093 11.6043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53427_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53427_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:22:52.06 -11:22:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 1.653 6303823590257238784 215.71728766490 -11.37233563934 12.0149 11.5302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53440_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53440_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:02:34.25 -14:21:25.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53472_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53472_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:46:16.77 -11:05:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.37, MAG_FAINT_SEARCH_LIMIT=11.35)GAIADR2_OUTPUT=# 0.201 6325601999321593344 221.56982336201 -11.09678189897 10.3783 9.9512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53554_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53554_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:35:14.33 -07:23:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 1.246 6331092853015837184 218.80989142166 -07.38654456388 11.7399 11.2166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53560_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
Preparing report for the candidate 53560_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
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Considering the candidate 53583_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53583_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:00:15.77 -13:36:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.624 6311907818219772032 225.06560890407 -13.61481048699 11.6989 10.9750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53617_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
Preparing report for the candidate 53617_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
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Considering the candidate 53649_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53649_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:02:37.71 -14:16:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.004 6301868422360730240 210.65739765671 -14.26677152392 11.8102 11.1659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53697_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
Preparing report for the candidate 53697_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
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Considering the candidate 53738_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53738_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:59:37.61 -10:37:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.813 6313912296636710656 224.90705919608 -10.61817261454 12.4732 11.7913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53751_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53751_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:53:06.27 -11:16:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.132 6313443354931101952 223.27655123866 -11.26759623632 12.9731 12.4870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53766_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53766_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:01:50.90 -08:05:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.345 6332330185849996672 225.46246021381 -08.09446449447 12.5608 12.0658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53784_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53784_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:05:04.10 -11:01:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.959 6312910645840112256 226.26687622728 -11.03308867266 12.7684 12.1995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53824_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53824_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:51:32.88 -13:57:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.281 6310526457954610432 222.88583059801 -13.96363317533 12.9068 12.3734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53825_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53825_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:38:27.13 -15:04:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.340 6286940662228284672 219.61342700727 -15.08226042890 12.6305 11.9276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53833_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53833_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:57:12.71 -14:08:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.376 6310378912942316928 224.30285516850 -14.13513646198 12.7792 12.1456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53834_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53834_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:17:59.22 -07:31:28.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53855_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53855_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:02:40.79 -05:36:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 1.405 6334023914793128576 225.66990018343 -05.60985832002 12.8143 12.2570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53860_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53860_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:58:54.62 -12:47:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.122 6312290933598997376 224.72745045800 -12.79352218982 12.9036 12.4036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53867_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53867_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:54:39.41 -10:20:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.993 6325898558223538944 223.66417906948 -10.34646957389 13.0970 12.5586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53887_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53887_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:05:38.49 -09:33:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.348 6320098595731150208 226.41018531968 -09.55338001366 13.3136 12.7590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53894_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53894_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:41:22.77 -06:27:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.564 6330896006074337280 220.34516203382 -06.46297796766 13.0438 12.4393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53910_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53910_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:17:11.28 -05:44:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.973 3640862159279292032 214.29720020606 -05.74534940084 12.9677 12.3829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53915_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53915_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:33:32.30 -15:00:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.172 6298909396052475648 218.38548036193 -15.00388192123 12.9892 12.3472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53922_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53922_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:03:15.59 -14:24:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.248 6301853849535643904 210.81538692723 -14.40766093127 12.6409 11.9607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53932_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53932_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:58:56.86 -14:30:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.456 6310295560512806528 224.73665396303 -14.51267569389 13.3403 12.6591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53940_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53940_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:02:17.65 -14:06:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.435 6302295582627822720 210.57395059781 -14.10682212186 12.8061 12.1941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53949_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
Preparing report for the candidate 53949_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
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Considering the candidate 53990_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53990_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:58:52.15 -11:29:03.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)
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Considering the candidate 53993_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53993_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:02:58.37 -14:10:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.269 6308818602863337344 225.74356175978 -14.17266773590 13.2788 12.3315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53999_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 53999_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:18:37.34 -07:01:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54007_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54007_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:01:17.17 -14:53:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 0.608 6307219092618433152 225.32162250897 -14.89221124175 13.2731 12.7749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54018_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54018_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:23:15.96 -06:31:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.789 3641442877513198592 215.81666000392 -06.52484525301 13.3184 12.7948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54039_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54039_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:30:48.91 -08:38:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.154 6328672243808383232 217.70438484535 -08.64149215822 13.5830 13.0792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54054_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54054_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:03:14.38 -14:08:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 0.681 6308819191274512640 225.80972221638 -14.13721020361 13.2000 12.5003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54077_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54077_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:03:18.07 -14:34:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 0.919 6308752597805189248 225.82528049741 -14.58000495824 13.1322 12.3738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54084_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54084_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:21:20.68 -11:23:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.895 6303832253207189888 215.33653766576 -11.39963073404 13.5547 13.0043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54086_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54086_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:55:09.92 -07:16:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54099_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54099_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:04:55.31 -13:39:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.327 6308962952419846656 226.23055162793 -13.66268889470 13.4828 13.0285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54107_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54107_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:03:10.50 -14:15:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.085 6308808574115343104 225.79416653989 -14.25230430848 13.2662 12.5525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54139_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54139_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:01:03.20 -15:05:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 0.440 6307207169789128704 225.26323207534 -15.08446236900 13.3894 12.8028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54161_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54161_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:04:49.77 -12:23:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.261 6312482317341710848 226.20773341049 -12.39431850343 13.5632 12.9986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54167_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
Preparing report for the candidate 54167_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
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Considering the candidate 54173_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
Preparing report for the candidate 54173_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
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Considering the candidate 54190_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54190_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:59:21.20 -15:02:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.880 6307236753523893760 224.83858220135 -15.03646095046 13.4891 12.8552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54211_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54211_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:01:08.52 -14:32:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.389 6308777100595088256 225.28577374144 -14.53766950212 13.4054 12.8581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54212_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54212_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:04:36.36 -13:15:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.869 6311984891409256576 226.15184322106 -13.25398086635 13.5451 13.0352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54215_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54215_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:04:33.98 -13:31:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.902 6308968690496178944 226.14146890003 -13.52099758239 13.5906 12.8698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54228_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54228_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:01:26.09 -14:32:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.151 6308776516479430528 225.35903541567 -14.54856688700 13.7138 13.1633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54229_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54229_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:04:09.62 -13:17:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.382 6311979359491468288 226.04044720677 -13.28676878408 13.6496 13.0470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54234_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54234_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:42:44.74 -08:43:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.569 6326979240714557312 220.68642425840 -08.73346350515 13.5121 12.7425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54235_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54235_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:05:50.14 -06:03:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.579 6333185434097879040 226.45961769815 -06.06405432940 13.9210 13.3352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54250_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54250_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:03:23.05 -13:06:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.702 6312044127598239872 225.84651045501 -13.10257203146 13.4731 12.7896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54254_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 54254_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:29:03.82 -06:12:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 0.456 3641328322146272256 217.26589676971 -06.20440279983 14.0532 13.5418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 25642_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
Preparing report for the candidate 25642_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
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Considering the candidate 04974_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 04974_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 14:28:45.15 -13:28:57.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 25997_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
Preparing report for the candidate 25997_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
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Considering the candidate 50050_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 50050_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
**** FOUND 15:03:27.96 -14:31:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 0.612 6308753147561002752 225.86654939875 -14.52880922531 12.5960 11.8301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 05170_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288
The candidate 05170_fd_Lib-01-Q1b1x1_2026-04-09_06-31-50_20.00sec_-4.90C_LIGHTs_0288 did not pass the final checks
