This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL
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 13.4280* 13 27 28.75 -04 53 09.4 10.6 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.9280,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4280 10.56CV 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 13.4280* 13 33 13.55 -08 09 06.7 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,2461143.9280,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4280 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4280* 13 44 29.84 -14 04 36.0 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,2461143.9280,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4280 11.98CV 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 13.4280* 13 22 02.73 -12 41 06.5 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,2461143.9280,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4280 12.01CV 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 13.4280* 14 04 05.10 -14 29 19.2 12.7 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,2461143.9280,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4280 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 13.4280* 14 11 25.03 -09 59 19.5 13.2 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,2461143.9280,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4280 13.20CV 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 13.4280* 14 08 27.93 -07 57 49.6 13.3 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.9280,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4280 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4280* 13 13 20.16 -09 58 55.5 11.5 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,2461143.9280,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4280 11.46CV 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 13.4280* 14 13 20.23 -12 34 26.3 12.3 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6303308022383772800,2461143.9280,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6303308022383772800 20260413.4280 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.90743030 27.02.2026 09:46:31.978 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
First image: 2461098.90743030 27.02.2026 09:46:31.978 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Last image: 2461143.92835470 13.04.2026 10:16:39.846 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.12
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5287
Objects passed selection criteria: 5262
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 3768.5
Average stars matched: 3694 (98.0231 %)
Memory usage VmPeak: 111316 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 05:26:44 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.90743030 27.02.2026 09:46:31.978 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
First image: 2461098.90743030 27.02.2026 09:46:31.978 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Last image: 2461143.92835470 13.04.2026 10:16:39.846 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 75
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 11 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): 28859
Objects passed selection criteria: 28806
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 22901.5
Average stars matched: 22146.8 (96.7044 %)
Memory usage VmPeak: 132316 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 05:27:44 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
SExtractor catalog cache: saved Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat to cache
SExtractor catalog cache: saved Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461143.92767653
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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits exists and is non-empty
Saving wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits to local_wcs_cache/
'wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> 'local_wcs_cache/wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits'
wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits exists and is non-empty
Saving wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits to local_wcs_cache/
'wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> 'local_wcs_cache/wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits'
wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits exists and is non-empty
Saving wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits to local_wcs_cache/
'wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits' -> 'local_wcs_cache/wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits'
wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits exists and is non-empty
Saving wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits to local_wcs_cache/
'wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits' -> 'local_wcs_cache/wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:42:50.965 -10:00:26.84
Second-epoch image center 13:42:37.622 -10:03:04.14
Angular distance between the image centers 0.0700 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 13:42:50.965 -10:00:26.84
Second-epoch image center 13:42:36.131 -10:03:35.63
Angular distance between the image centers 0.0803 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 13:42:37.622 -10:03:04.14
Second-epoch second image center 13:42:36.131 -10:03:35.63
Angular distance between the image centers 0.01067 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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits &> /tmp/tmp.8BTqyNknJ0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits &> /tmp/tmp.x91ptvp745
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits &> /tmp/tmp.BWKg7rIYGp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits &> /tmp/tmp.ncEFFXE6uT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
Found non-empty wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
The reference image (wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits) and catalog (wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat) found
'wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat' -> 'wcsmag.cat'
Read 5441 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6102 to 213.7377 deg, Dec -15.2798 to -4.6610 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 197.6102 to 213.7377 deg, Dec -15.2798 to -4.6610 deg
Loaded 4386 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): 3481 out of 3580 total matches.
Matched with Tycho-2 3580 out of 5441 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.932009
a=0.000000 b=1.000000 c=22.932009
From vast_summary.log: estimated ref. image limiting mag.: -8.12
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.81
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.81
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
2.4 pix Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
2.3 pix fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
2.3 pix fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
Limiting magnitude estimates:
14.8 mag. Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
14.8 mag. Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
13.2 mag. fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
13.1 mag. fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.7 (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.8BTqyNknJ0 (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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> 'wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS-calibrated image found: wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Checking if the catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS catalog name: wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=359, passed=5441
Got 5441 stars (including 5082 good ones) from the SExtractor catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
util/solve_plate_with_UCAC5 got 5441 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits -region wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.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.x91ptvp745 (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-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.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-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.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-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> 'wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS-calibrated image found: wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Checking if the catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS catalog name: wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=377, passed=5451
Got 5451 stars (including 5071 good ones) from the SExtractor catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat
util/solve_plate_with_UCAC5 got 5451 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5400 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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits -region wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BWKg7rIYGp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
Checking if the catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat corresponding to the image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat corresponding to the image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
WCS catalog name: wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=122, passed=2155
Got 2155 stars (including 2031 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat
util/solve_plate_with_UCAC5 got 2155 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 2136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 2138 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 2138 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits -region wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.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.ncEFFXE6uT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
Checking if the catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat corresponding to the image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat corresponding to the image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
WCS catalog name: wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=119, passed=2123
Got 2123 stars (including 2000 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat
util/solve_plate_with_UCAC5 got 2123 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 2102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 2102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 2102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits -region wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits'
Saving fully-calibrated image wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits'
Saving fully-calibrated image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits'
Saving fully-calibrated image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits'
Preparing the HTML report for the field Vir-12-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20264.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20205_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 20205_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:14.32 -14:14:32.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20230_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 20230_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:10:21.32 -13:18:14.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20251_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 20251_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:10:33.27 -14:06:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20257_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 20257_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:12:42.79 -14:17:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20264_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
Preparing report for the candidate 20264_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Vir-12-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:27:28.75 -04:53:09.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
SExtractor catalog cache: saved Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat to cache
SExtractor catalog cache: saved Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Creating symlink local_wcs_cache/wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits exists and is non-empty
wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits exists and is non-empty
wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits exists and is non-empty
wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:42:50.965 -10:00:26.84
Second-epoch image center 13:42:37.622 -10:03:04.14
Angular distance between the image centers 0.0700 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 13:42:50.965 -10:00:26.84
Second-epoch image center 13:42:36.131 -10:03:35.63
Angular distance between the image centers 0.0803 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 13:42:37.622 -10:03:04.14
Second-epoch second image center 13:42:36.131 -10:03:35.63
Angular distance between the image centers 0.01067 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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits &> /tmp/tmp.rhiPUCf75P
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits &> /tmp/tmp.tQc2VqMsaU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits &> /tmp/tmp.AU3UUWfMpT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits &> /tmp/tmp.IiWVyo0TvH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
Found non-empty wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
The reference image (wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits) and catalog (wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat) found
'wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat' -> 'wcsmag.cat'
Read 31003 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6003 to 213.7472 deg, Dec -15.2838 to -4.6412 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 197.6003 to 213.7472 deg, Dec -15.2838 to -4.6412 deg
Loaded 4397 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): 3514 out of 3762 total matches.
Matched with Tycho-2 3762 out of 31003 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.792651
a=0.000000 b=1.000000 c=22.792651
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.94
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.94
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 59 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
2.3 pix Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
2.1 pix fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
2.2 pix fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
Limiting magnitude estimates:
14.9 mag. Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
14.9 mag. Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
13.6 mag. fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
13.6 mag. fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.2 (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.rhiPUCf75P (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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> 'wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS-calibrated image found: wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Checking if the catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS catalog name: wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1266, passed=30996
Got 30996 stars (including 29698 good ones) from the SExtractor catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
util/solve_plate_with_UCAC5 got 30996 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 30629 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 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 30629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 30629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits -region wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.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.tQc2VqMsaU (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-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.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-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.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-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> 'wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS-calibrated image found: wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Checking if the catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS catalog name: wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1340, passed=30816
Got 30816 stars (including 29439 good ones) from the SExtractor catalog wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat
util/solve_plate_with_UCAC5 got 30816 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
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(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 30434 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 373 to 428 (Dec -15.3 to -4.6)
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(), 30433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 30433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits -region wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AU3UUWfMpT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
Checking if the catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat corresponding to the image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat corresponding to the image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
WCS catalog name: wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=375, passed=15470
Got 15470 stars (including 15068 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat
util/solve_plate_with_UCAC5 got 15470 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 15375 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 15376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 15376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits -region wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.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.IiWVyo0TvH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
Checking if the catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat corresponding to the image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat corresponding to the image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
WCS catalog name: wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=354, passed=15062
Got 15062 stars (including 14683 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat
util/solve_plate_with_UCAC5 got 15062 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 14983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 14983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 14983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits -region wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.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-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/wcs_Vir-12-Q1b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Saving fully-calibrated image wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/wcs_Vir-12-Q1b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Saving fully-calibrated image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-15-41_20.00sec_-4.90C_LIGHTs_0189.fits
Saving fully-calibrated image wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-12-Q1b1x1_051744_TTUQ1b1x1_8225_Chd099fL/wcs_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190.fits
Preparing the HTML report for the field Vir-12-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out00703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out02399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out03325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out04382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out50029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out50048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out50052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out50053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out50059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out50060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52784.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 25s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 52265_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52265_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52267_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52267_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:24:31.97 -09:03:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52268_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52268_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:12:27.44 -08:27:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52272_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52272_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:14.34 -14:14:32.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52319_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52319_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:10:33.28 -14:06:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52330_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52330_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:12:42.82 -14:17:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52333_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52333_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:27:28.75 -04:53:09.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52337_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52337_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:14.18 -13:50:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52375_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52375_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:03.16 -14:23:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52391_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52391_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:13:32.78 -14:25:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52397_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52397_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:13:20.56 -14:28:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52417_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52417_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:00.09 -14:04:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52420_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52420_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:21.85 -14:21:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52439_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52439_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:09:34.19 -14:44:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52443_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52443_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:43:01.86 -15:06:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52462_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
Preparing report for the candidate 52462_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
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Considering the candidate 52464_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52464_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:14:13.23 -14:32:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 1.217 3608728347841928960 198.55546221747 -14.54833829498 11.7673 11.2282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52467_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52467_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:12:28.66 -14:18:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52480_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52480_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:10:55.15 -13:49:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52482_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52482_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:12:12.59 -14:20:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52489_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52489_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:52.22 -14:21:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52504_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52504_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:13:49.46 -14:31:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52506_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52506_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:49.41 -13:46:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52508_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
Preparing report for the candidate 52508_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
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Considering the candidate 52512_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52512_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:10:32.72 -13:54:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52520_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52520_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:57.45 -14:20:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52524_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52524_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:10:26.20 -14:28:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.830 3608849264057159168 197.60968946333 -14.47204653535 12.2301 11.8234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52537_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52537_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:08.00 -14:01:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52541_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52541_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:40.91 -13:53:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52553_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52553_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:11.66 -13:59:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52556_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
Preparing report for the candidate 52556_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
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Considering the candidate 52661_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52661_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:13:37.03 -14:23:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52664_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52664_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:13:28.80 -14:31:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52665_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52665_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:28.63 -14:20:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52668_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
Preparing report for the candidate 52668_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
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Considering the candidate 52678_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52678_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:35:27.38 -04:55:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52700_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52700_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:13:04.77 -11:04:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52707_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52707_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:35:52.69 -07:21:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52725_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52725_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:11:54.62 -14:19:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52741_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
Preparing report for the candidate 52741_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
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Considering the candidate 52764_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52764_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:10:37.13 -13:49:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52784_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
Preparing report for the candidate 52784_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
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Considering the candidate 52826_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52826_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:14:46.10 -14:23:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52853_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 52853_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 13:36:14.47 -08:05:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.291 3630478130948383232 204.06093166482 -08.09838630541 13.8133 13.2584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 04382_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 04382_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:12:09.90 -13:31:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.364 6303095855294247552 213.04134300551 -13.52003808289 12.1614 11.5872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50060_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 50060_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:11:46.73 -14:28:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 1.128 6301322205599687808 212.94478862663 -14.48236326016 11.5824 10.9478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50059_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 50059_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:10:17.98 -13:41:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 0.314 6301588317477846016 212.57500030827 -13.69944855138 11.7081 11.1983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50053_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 50053_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:11:19.26 -14:10:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.431 6301367766612847616 212.83033409423 -14.17702327320 12.0736 11.4388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50052_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 50052_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:11:14.79 -14:54:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.823 6301164425681278848 212.81153160371 -14.90595672153 12.3277 11.7225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50048_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 50048_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:13:00.90 -14:12:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.543 6301355736408523520 213.25405043102 -14.21178650984 12.5005 11.7583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50029_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 50029_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:10:39.47 -14:03:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.549 6301558222642528384 212.66483778095 -14.06005513024 13.1291 12.3960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 14682_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
Preparing report for the candidate 14682_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
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Considering the candidate 01876_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 01876_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:10:17.67 -14:29:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02399_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 02399_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:11:21.19 -14:15:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.742 6301363845307335936 212.83848370688 -14.26469991929 12.0774 11.5636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 00703_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 00703_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:10:16.81 -14:56:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.783 6301166105013379456 212.56970427862 -14.93921049275 12.6119 12.1527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 05010_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 05010_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:10:21.31 -13:18:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07139_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
Preparing report for the candidate 07139_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
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Considering the candidate 03325_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 03325_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
**** FOUND 14:10:03.14 -13:55:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 0.411 6301575539950641280 212.51307191948 -13.92344701670 12.6688 12.1222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 10147_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190
The candidate 10147_fd_Vir-12-Q1b1x1_2026-04-13_05-16-39_20.00sec_-4.90C_LIGHTs_0190 did not pass the final checks
