This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD
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
VARIABLE_NAME,2461143.9401,11.38,0.05,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 20260413.4401 11.38CV 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,2461143.9401,11.71,0.05,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 20260413.4401 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461143.9401,12.12,0.05,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 20260413.4401 12.12CV 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,2461143.9401,12.59,0.05,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 20260413.4401 12.59CV 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
SX Lib,2461143.9401,9.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SX Lib 20260413.4401 9.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GI Lib,2461143.9401,12.11,0.05,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
GI Lib 20260413.4401 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 J145520-1705.1,2461143.9401,12.38,0.05,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 J145520-1705.1 20260413.4401 12.38CV 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
RZ Lib,2461143.9401,12.21,0.05,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
RZ Lib 20260413.4401 12.21CV 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: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
First image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Last image: 2461143.94049676 13.04.2026 10:34:08.920 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.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.: -8.31
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6352
Objects passed selection criteria: 6326
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 4426.25
Average stars matched: 4321.25 (97.6278 %)
Memory usage VmPeak: 112316 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 05:36:10 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: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
First image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Last image: 2461143.94049676 13.04.2026 10:34:08.920 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 57
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.03
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: 17 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): 39398
Objects passed selection criteria: 39323
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 30690.2
Average stars matched: 29537.8 (96.2447 %)
Memory usage VmPeak: 141872 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 05:37:13 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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
SExtractor catalog cache: saved Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.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: 2461143.93978285
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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits exists and is non-empty
Saving wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits to local_wcs_cache/
'wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits' -> 'local_wcs_cache/wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits'
wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits exists and is non-empty
Saving wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits to local_wcs_cache/
'wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits' -> 'local_wcs_cache/wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.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 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:28.551 -18:01:38.53
Angular distance between the image centers 0.1413 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 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:27.653 -18:02:23.90
Angular distance between the image centers 0.1461 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 15:06:28.551 -18:01:38.53
Second-epoch second image center 15:06:27.653 -18:02:23.90
Angular distance between the image centers 0.01310 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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.viHxPHitwl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.eMu6HPQ9Dl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits &> /tmp/tmp.eXvCUvANCe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits &> /tmp/tmp.aCFNA5Evpm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
Found non-empty wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
The reference image (wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits) and catalog (wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat) found
'wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat' -> 'wcsmag.cat'
Read 6705 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 218.3309 to 235.1834 deg, Dec -23.2849 to -12.5918 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 218.3309 to 235.1834 deg, Dec -23.2849 to -12.5918 deg
Loaded 6143 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): 4648 out of 4760 total matches.
Matched with Tycho-2 4760 out of 6705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.875304
a=0.000000 b=1.000000 c=22.875304
From vast_summary.log: estimated ref. image limiting mag.: -8.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.57
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:
2.4 pix Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
2.4 pix Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
2.3 pix fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
2.3 pix fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
Limiting magnitude estimates:
14.6 mag. Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
14.6 mag. Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
13.1 mag. fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
12.8 mag. fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.5 (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.viHxPHitwl (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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=403, passed=6705
Got 6705 stars (including 6294 good ones) from the SExtractor catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 6705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6639 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6637 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6637 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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.eMu6HPQ9Dl (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-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=425, passed=6649
Got 6649 stars (including 6218 good ones) from the SExtractor catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 6649 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6581 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6581 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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.eXvCUvANCe (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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
Checking if the catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat corresponding to the image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat corresponding to the image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
WCS catalog name: wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=129, passed=2360
Got 2360 stars (including 2227 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat
util/solve_plate_with_UCAC5 got 2360 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 390 (Dec -23.6 to -12.2)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2323 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 390 (Dec -23.6 to -12.2)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2323 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2323 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits -region wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.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.aCFNA5Evpm (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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
Checking if the catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat corresponding to the image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat corresponding to the image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
WCS catalog name: wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=123, passed=2086
Got 2086 stars (including 1961 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat
util/solve_plate_with_UCAC5 got 2086 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 390 (Dec -23.7 to -12.2)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 390 (Dec -23.7 to -12.2)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits -region wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
Saving fully-calibrated image wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
Saving fully-calibrated image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits'
Saving fully-calibrated image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits'
Preparing the HTML report for the field Lib-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20387.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 20334_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 20334_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:34:26.70 -22:23:28.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20370_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 20370_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:33:55.12 -22:18:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.23, MAG_FAINT_SEARCH_LIMIT=11.21)GAIADR2_OUTPUT=# 1.572 6279309020739471104 218.48010061333 -22.30727277157 9.6803 9.2049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20387_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 20387_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:33:52.79 -22:05:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.59, MAG_FAINT_SEARCH_LIMIT=11.57)GAIADR2_OUTPUT=# 1.291 6279365027113066368 218.47033957318 -22.09893816623 10.1485 9.8569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05160_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 05160_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:33:16.40 -15:19:35.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Lib-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
SExtractor catalog cache: saved Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits exists and is non-empty
wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.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 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:28.551 -18:01:38.53
Angular distance between the image centers 0.1413 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 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:27.653 -18:02:23.90
Angular distance between the image centers 0.1461 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 15:06:28.551 -18:01:38.53
Second-epoch second image center 15:06:27.653 -18:02:23.90
Angular distance between the image centers 0.01310 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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.4KsCqP1Hfd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.3RCcJwvAK5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits &> /tmp/tmp.Z9lTXloZrW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits &> /tmp/tmp.6e1iS2BYBv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
Found non-empty wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
The reference image (wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits) and catalog (wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat) found
'wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat' -> 'wcsmag.cat'
Read 42407 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 218.2429 to 235.1834 deg, Dec -23.2935 to -12.5730 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 218.2429 to 235.1834 deg, Dec -23.2935 to -12.5730 deg
Loaded 6189 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): 4998 out of 5340 total matches.
Matched with Tycho-2 5340 out of 42407 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.714492
a=0.000000 b=1.000000 c=22.714492
From vast_summary.log: estimated ref. image limiting mag.: -8.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.68
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
2.3 pix Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
2.1 pix fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
2.2 pix fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
Limiting magnitude estimates:
14.7 mag. Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
14.7 mag. Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
13.5 mag. fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
13.3 mag. fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 12.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.4KsCqP1Hfd (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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1940, passed=42395
Got 42395 stars (including 40408 good ones) from the SExtractor catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 42395 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42005 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42005 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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.3RCcJwvAK5 (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-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1927, passed=42819
Got 42819 stars (including 40844 good ones) from the SExtractor catalog wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 42819 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 42410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 42409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 42409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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.Z9lTXloZrW (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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
Checking if the catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat corresponding to the image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat corresponding to the image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
WCS catalog name: wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=461, passed=20398
Got 20398 stars (including 19909 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat
util/solve_plate_with_UCAC5 got 20398 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 20190 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 20190 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 20190 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits -region wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.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.6e1iS2BYBv (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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
Checking if the catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat corresponding to the image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat corresponding to the image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
WCS catalog name: wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=463, passed=18266
Got 18266 stars (including 17774 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat
util/solve_plate_with_UCAC5 got 18266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.7 to -12.1)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 18049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.7 to -12.1)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 18048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 18049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits -region wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.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-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/wcs_Lib-03-Q1b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Saving fully-calibrated image wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/wcs_Lib-03-Q1b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Saving fully-calibrated image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-33-07_20.00sec_-4.90C_LIGHTs_0205.fits
Saving fully-calibrated image wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.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_2026-04-13_CI_Lib-03-Q1b1x1_053459_TTUQ1b1x1_25821_Xh8lTyLD/wcs_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206.fits
Preparing the HTML report for the field Lib-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out10485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54076.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 53692_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 53692_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:25:27.94 -15:10:45.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)
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Considering the candidate 53693_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 53693_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:25:24.62 -16:02:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.781 6259595838109495552 231.35243737634 -16.03947350256 12.0619 11.6424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53694_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 53694_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:26:35.80 -14:10:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53695_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 53695_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:17:39.32 -17:12:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.52, MAG_FAINT_SEARCH_LIMIT=11.50)GAIADR2_OUTPUT=# 0.520 6258999357347770240 229.41368897805 -17.20290439442 10.5156 10.0729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53757_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 53757_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:33:52.79 -22:05:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.24, MAG_FAINT_SEARCH_LIMIT=11.22)GAIADR2_OUTPUT=# 1.278 6279365027113066368 218.47033957318 -22.09893816623 10.1485 9.8569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53764_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 53764_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:34:13.74 -21:52:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.29, MAG_FAINT_SEARCH_LIMIT=11.27)GAIADR2_OUTPUT=# 1.303 6279395706063043584 218.55760391241 -21.87640356628 10.1586 9.9100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53766_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 53766_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:33:22.13 -22:19:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.33, MAG_FAINT_SEARCH_LIMIT=11.31)GAIADR2_OUTPUT=# 1.124 6279307989947611904 218.34253888190 -22.32918647147 10.1743 9.7143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53787_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 53787_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:33:36.86 -22:06:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 1.129 6279359254677020800 218.40390473795 -22.11598495587 10.5800 10.2525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53820_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 53820_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:38:09.58 -16:32:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53838_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
Preparing report for the candidate 53838_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
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Considering the candidate 53916_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
Preparing report for the candidate 53916_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
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Considering the candidate 54005_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54005_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:35:00.68 -21:03:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54014_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
Preparing report for the candidate 54014_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
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Considering the candidate 54021_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54021_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:27:36.13 -19:10:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 2.423 6254817193078552832 231.89990621470 -19.16727665839 12.2066 11.4310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54048_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54048_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:33:19.20 -21:51:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 1.203 6279384917105195904 218.33035572251 -21.86594766271 11.8394 11.2546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54076_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
Preparing report for the candidate 54076_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
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Considering the candidate 54102_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54102_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:32:45.43 -20:17:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54118_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54118_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:35:58.34 -22:15:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.202 6279321042352266240 218.99275104296 -22.25756450272 12.2120 11.7248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54123_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54123_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:50:34.77 -16:00:52.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54149_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54149_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:33:35.26 -21:27:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.354 6279608500219174016 218.39731983303 -21.46352551588 12.0962 11.5697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54151_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54151_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:48:59.31 -12:41:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 0.462 6311688126348904576 222.24725659325 -12.68978032263 12.7053 12.1599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54212_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54212_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:25:19.49 -17:04:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 2.937 6258629302965802624 231.33134145300 -17.07647184469 12.6621 11.8316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54220_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54220_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:35:43.27 -22:03:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.370 6279339802769405184 218.93021379838 -22.06212880228 12.1747 11.6936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54253_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54253_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:49:26.36 -12:41:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.735 6311708639112701696 222.35993235357 -12.69220771069 12.8284 12.1569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54321_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54321_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:35:27.91 -22:06:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.662 6279338226517305344 218.86647807409 -22.10006316199 12.3292 11.8946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54344_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54344_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 14:49:22.64 -12:41:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.609 6311708639112702592 222.34437138026 -12.69222047070 13.1005 12.6449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54385_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 54385_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:32:30.89 -22:26:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10485_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
Preparing report for the candidate 10485_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
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Considering the candidate 23565_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
Preparing report for the candidate 23565_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
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Considering the candidate 03573_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 03573_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:35:33.15 -22:07:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24851_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
Preparing report for the candidate 24851_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
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Considering the candidate 06273_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 06273_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:38:03.68 -21:22:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38067_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
Preparing report for the candidate 38067_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
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Considering the candidate 51116_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 51116_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:37:48.04 -16:09:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31794_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 31794_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:33:16.40 -15:19:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12620_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 12620_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
**** FOUND 15:12:13.08 -19:47:28.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 40862_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206
The candidate 40862_fd_Lib-03-Q1b1x1_2026-04-13_05-34-08_20.00sec_-4.90C_LIGHTs_0206 did not pass the final checks
