This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2558* 11 46 07.19 +01 03 04.4 9.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7558,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2558 9.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2558* 12 19 44.50 -05 35 54.1 12.0 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7558,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2558 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2558* 12 05 59.13 +00 14 50.2 12.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7558,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2558 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!
TCP 2026 04 09.2558* 12 12 50.25 -02 46 49.3 13.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7558,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2558 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2558* 11 54 32.08 -05 48 44.6 13.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7558,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2558 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2558* 12 26 32.89 +01 31 47.3 14.0 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7558,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2558 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2558* 12 17 03.08 -02 19 26.3 14.1 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7558,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2558 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2558* 12 03 58.65 -01 19 12.1 14.8 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7558,14.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2558 14.80CV 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: 2461093.86218641 22.02.2026 08:41:22.906 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
First image: 2461093.86218641 22.02.2026 08:41:22.906 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
Last image: 2461139.75607392 09.04.2026 06:08:34.787 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.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.: -7.74
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4431
Objects passed selection criteria: 4429
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 4280
Average stars matched: 4180.5 (97.6752 %)
Memory usage VmPeak: 110912 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:22:45 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: 2461093.86218641 22.02.2026 08:41:22.906 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
First image: 2461093.86218641 22.02.2026 08:41:22.906 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
Last image: 2461139.75607392 09.04.2026 06:08:34.787 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 43
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.40
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 26127
Objects passed selection criteria: 26054
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 25246.8
Average stars matched: 24313 (96.3015 %)
Memory usage VmPeak: 130072 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:23:42 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
SExtractor catalog cache: saved Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat to cache
SExtractor catalog cache: saved Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461139.75545164
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_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits exists and is non-empty
Saving wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits to local_wcs_cache/
'wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits' -> 'local_wcs_cache/wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits'
wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits exists and is non-empty
Saving wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits to local_wcs_cache/
'wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits' -> 'local_wcs_cache/wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits'
wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits exists and is non-empty
Saving wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits to local_wcs_cache/
'wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits' -> 'local_wcs_cache/wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits'
wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits exists and is non-empty
Saving wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits to local_wcs_cache/
'wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits' -> 'local_wcs_cache/wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:59.773 -02:00:02.82
Second-epoch image center 12:00:18.398 -01:58:27.92
Angular distance between the image centers 0.0819 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 11:59:59.773 -02:00:02.82
Second-epoch image center 12:00:21.356 -01:58:09.05
Angular distance between the image centers 0.0953 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 12:00:18.398 -01:58:27.92
Second-epoch second image center 12:00:21.356 -01:58:09.05
Angular distance between the image centers 0.01339 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits &> /tmp/tmp.hCgsuy01zB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits &> /tmp/tmp.Fv2EqquBHo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits &> /tmp/tmp.dNUx4EX8XI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits &> /tmp/tmp.OTlA9ra6x9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits and wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits and wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat
Found non-empty wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits and wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat
The reference image (wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits) and catalog (wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat) found
'wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat' -> 'wcsmag.cat'
Read 5852 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 172.0998 to 187.9210 deg, Dec -7.2990 to +3.3108 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 172.0998 to 187.9210 deg, Dec -7.2990 to 3.3108 deg
Loaded 3755 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): 3122 out of 3271 total matches.
Matched with Tycho-2 3271 out of 5852 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.884713
a=0.000000 b=1.000000 c=22.884713
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.14
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.14
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:
2.3 pix Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
2.3 pix Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
2.4 pix fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
2.4 pix fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
Limiting magnitude estimates:
15.1 mag. Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
15.1 mag. Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
15.1 mag. fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
15.1 mag. fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hCgsuy01zB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits' -> 'wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
WCS-calibrated image found: wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
Checking if the catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat corresponding to the image wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat corresponding to the image wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
WCS catalog name: wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=443, passed=5852
Got 5852 stars (including 5404 good ones) from the SExtractor catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat
util/solve_plate_with_UCAC5 got 5852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 5821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 5820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 5820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits -region wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.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.Fv2EqquBHo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits' -> 'wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
WCS_IMAGE_NAME=wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
WCS-calibrated image found: wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
Checking if the catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat corresponding to the image wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits alredy exist and is non-empty...
Catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat corresponding to the image wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
WCS catalog name: wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=442, passed=5811
Got 5811 stars (including 5362 good ones) from the SExtractor catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat
util/solve_plate_with_UCAC5 got 5811 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits -region wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.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.dNUx4EX8XI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
WCS-calibrated image found: wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
Checking if the catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
WCS catalog name: wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=367, passed=5721
Got 5721 stars (including 5342 good ones) from the SExtractor catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat
util/solve_plate_with_UCAC5 got 5721 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 5701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 5700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 5700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits -region wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.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.OTlA9ra6x9 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
WCS_IMAGE_NAME=wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
WCS-calibrated image found: wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
Checking if the catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat corresponding to the image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat corresponding to the image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
WCS catalog name: wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=372, passed=5710
Got 5710 stars (including 5337 good ones) from the SExtractor catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat
util/solve_plate_with_UCAC5 got 5710 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5691 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5690 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5690 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits -region wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits'
Saving fully-calibrated image wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits'
Saving fully-calibrated image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits'
Saving fully-calibrated image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits'
Preparing the HTML report for the field Vir-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20221.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 2s
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Considering the candidate 20211_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
Preparing report for the candidate 20211_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
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Considering the candidate 20212_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 20212_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:27:01.89 -03:32:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20221_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
Preparing report for the candidate 20221_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
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Considering the candidate 20223_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 20223_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:22:52.80 +01:17:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.339 3700131612748704000 185.71992293689 +01.29752900391 12.5848 12.2075 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Vir-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:46:07.19 +01:03:04.4
12:19:44.50 -05:35:54.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
SExtractor catalog cache: saved Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat to cache
SExtractor catalog cache: saved Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
Creating symlink local_wcs_cache/wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits exists and is non-empty
wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits exists and is non-empty
wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits exists and is non-empty
wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:59.773 -02:00:02.82
Second-epoch image center 12:00:18.398 -01:58:27.92
Angular distance between the image centers 0.0819 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 11:59:59.773 -02:00:02.82
Second-epoch image center 12:00:21.356 -01:58:09.05
Angular distance between the image centers 0.0953 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 12:00:18.398 -01:58:27.92
Second-epoch second image center 12:00:21.356 -01:58:09.05
Angular distance between the image centers 0.01339 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits &> /tmp/tmp.u5H1IDNHMo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits &> /tmp/tmp.d5twsIVLED
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits &> /tmp/tmp.ziSr4qcRJu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits &> /tmp/tmp.RJwGpLycdF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits and wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits and wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat
Found non-empty wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits and wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat
The reference image (wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits) and catalog (wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat) found
'wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat' -> 'wcsmag.cat'
Read 32492 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 172.0947 to 187.9493 deg, Dec -7.3038 to +3.3170 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 172.0947 to 187.9493 deg, Dec -7.3038 to 3.3170 deg
Loaded 3770 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): 3039 out of 3314 total matches.
Matched with Tycho-2 3314 out of 32492 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.740798
a=0.000000 b=1.000000 c=22.740798
From vast_summary.log: estimated ref. image limiting mag.: -7.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
2.1 pix Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
2.2 pix fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
2.2 pix fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
Limiting magnitude estimates:
15.3 mag. Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
15.3 mag. Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
15.3 mag. fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
15.3 mag. fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.u5H1IDNHMo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits' -> 'wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
WCS-calibrated image found: wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
Checking if the catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat corresponding to the image wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat corresponding to the image wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
WCS catalog name: wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1375, passed=32479
Got 32479 stars (including 31051 good ones) from the SExtractor catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat
util/solve_plate_with_UCAC5 got 32479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 32410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 32410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 32410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits -region wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.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.d5twsIVLED (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits' -> 'wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
WCS_IMAGE_NAME=wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
WCS-calibrated image found: wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
Checking if the catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat corresponding to the image wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits alredy exist and is non-empty...
Catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat corresponding to the image wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
WCS catalog name: wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1376, passed=32478
Got 32478 stars (including 31045 good ones) from the SExtractor catalog wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat
util/solve_plate_with_UCAC5 got 32478 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 32312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 32312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 32312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits -region wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.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.ziSr4qcRJu (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
WCS-calibrated image found: wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
Checking if the catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
WCS catalog name: wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1401, passed=30164
Got 30164 stars (including 28733 good ones) from the SExtractor catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat
util/solve_plate_with_UCAC5 got 30164 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 30063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 30062 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 30062 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits -region wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.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.RJwGpLycdF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
WCS_IMAGE_NAME=wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
WCS-calibrated image found: wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
Checking if the catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat corresponding to the image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat corresponding to the image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
WCS catalog name: wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1484, passed=30377
Got 30377 stars (including 28855 good ones) from the SExtractor catalog wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat
util/solve_plate_with_UCAC5 got 30377 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 30264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 30264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 30264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits -region wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/wcs_Vir-06-Q2b1x1_2026-02-22_02-41-22_20.00sec_-14.90C_LIGHT_0411.fits
Saving fully-calibrated image wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/wcs_Vir-06-Q2b1x1_2026-02-22_02-42-10_20.00sec_-14.90C_LIGHT_0412.fits
Saving fully-calibrated image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-07-41_20.00sec_-4.90C_LIGHT_0214.fits
Saving fully-calibrated image wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-06-Q2b1x1_011931_TTUQ2b1x1_24064_WUNpvCy8/wcs_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215.fits
Preparing the HTML report for the field Vir-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52248.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52252.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 52059_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52059_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 11:59:23.00 +00:56:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.133 3891240065234767488 179.84568342985 +00.94508426420 14.4974 13.9206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52074_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52074_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 11:46:07.19 +01:03:04.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52085_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52085_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:19:44.50 -05:35:54.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52086_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52086_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:03:31.88 -02:25:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52095_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
Preparing report for the candidate 52095_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
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Considering the candidate 52123_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52123_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:03:05.18 -01:38:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52133_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
Preparing report for the candidate 52133_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
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Considering the candidate 52138_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52138_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 11:56:59.84 +00:37:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52140_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52140_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:26:14.26 +00:32:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52141_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
Preparing report for the candidate 52141_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
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Considering the candidate 52148_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52148_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 11:50:31.96 -02:24:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52164_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52164_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 11:59:07.25 -04:46:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52174_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52174_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 11:49:47.25 -04:51:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52183_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52183_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:11:56.25 -00:28:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52187_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
Preparing report for the candidate 52187_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
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Considering the candidate 52190_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52190_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:13:40.96 +01:52:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52193_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
Preparing report for the candidate 52193_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
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Considering the candidate 52197_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52197_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:06:58.09 -05:02:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52216_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52216_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 11:56:52.40 -02:35:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52218_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52218_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 11:58:06.98 +00:52:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52227_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52227_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 11:51:06.36 +01:47:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52239_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52239_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:27:12.81 -03:28:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 1.587 3693144594311797760 186.80298739238 -03.48285034466 14.5611 13.7224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52244_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52244_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:03:44.51 +01:06:13.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)
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Considering the candidate 52246_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52246_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:26:06.73 -01:26:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 2.075 3694796919769763712 186.52751108787 -01.43944807179 14.7995 14.3149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52247_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52247_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:06:23.49 +02:14:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52248_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52248_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:00:23.90 +00:29:28.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)
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Considering the candidate 52252_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
Preparing report for the candidate 52252_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
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Considering the candidate 52253_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52253_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:12:32.66 +00:46:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.669 3699212661545873280 183.13646703714 +00.78159346467 14.7513 14.1409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52256_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52256_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
**** FOUND 12:15:36.04 -01:01:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.75, MAG_FAINT_SEARCH_LIMIT=15.73)GAIADR2_OUTPUT=# 4.386 3697661388078573952 183.90121491997 -01.02648247853 14.0667 12.9263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52270_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215
The candidate 52270_fd_Vir-06-Q2b1x1_2026-04-09_01-08-34_20.00sec_-4.90C_LIGHT_0215 did not pass the final checks
