This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8
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 19.2701* 13 39 59.28 -13 17 24.7 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,2461149.7701,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.2701 12.02CV 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 19.2701* 13 27 47.29 -07 42 18.2 12.3 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.7701,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.2701 12.32CV 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 19.2701* 13 17 17.74 -11 58 25.5 12.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.7701,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.2701 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 19.2701* 13 58 57.62 -14 06 28.7 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,2461149.7701,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.2701 12.72CV 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 19.2701* 13 39 19.58 -10 01 29.9 14.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.7701,14.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.2701 14.42CV 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 19.2701* 13 35 53.52 -13 18 53.6 14.5 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,2461149.7701,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.2701 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Last image: 2461149.77039516 19.04.2026 06:29:12.142 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.09
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): 4407
Objects passed selection criteria: 4407
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 4267.75
Average stars matched: 4112.5 (96.3623 %)
Memory usage VmPeak: 110848 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 01:32:47 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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Last image: 2461149.77039516 19.04.2026 06:29:12.142 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 67
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.80
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: 14 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): 26071
Objects passed selection criteria: 26011
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 25155.8
Average stars matched: 24002.2 (95.4146 %)
Memory usage VmPeak: 129976 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 01:33:39 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat to cache
SExtractor catalog cache: saved Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.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: 2461149.76982917
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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits exists and is non-empty
Saving wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits to local_wcs_cache/
'wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> 'local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits'
wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits exists and is non-empty
Saving wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits to local_wcs_cache/
'wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> 'local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits'
wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits exists and is non-empty
Saving wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits to local_wcs_cache/
'wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits' -> 'local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits'
wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits exists and is non-empty
Saving wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits to local_wcs_cache/
'wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits' -> 'local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits (1st reference image)
verification OK: wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Image size: 937.3'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:50.965 -10:00:26.84 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits (1st new image)
verification OK: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:54.357 -09:56:13.90 J2000 4789.000 3195.000
###################################
###################################
# 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 13:42:54.357 -09:56:13.90
Angular distance between the image centers 0.0716 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits (2nd new image)
verification OK: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
Image size: 937.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:52.646 -09:56:54.02 J2000 4789.000 3195.000
###################################
###################################
# 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 13:42:52.646 -09:56:54.02
Angular distance between the image centers 0.0595 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 13:42:54.357 -09:56:13.90
Second-epoch second image center 13:42:52.646 -09:56:54.02
Angular distance between the image centers 0.01317 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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits &> /tmp/tmp.k8VwYmEk7Y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits &> /tmp/tmp.qVGbslu81A
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits &> /tmp/tmp.58EmTIbgYp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits &> /tmp/tmp.5C2GrYfe9m
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
Found non-empty wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
The reference image (wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits) and catalog (wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat) found
'wcs_Vir-12-Q2b1x1_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 22.918872
a=0.000000 b=1.000000 c=22.918872
From vast_summary.log: estimated ref. image limiting mag.: -8.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.83
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.83
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
2.4 pix Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
2.6 pix fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
2.6 pix fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
Limiting magnitude estimates:
14.8 mag. Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
14.8 mag. Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
14.8 mag. fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
14.9 mag. fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (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.k8VwYmEk7Y (6) ############
Parsing command line arguments...
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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/util/wcs_image_calibration.sh: line 129: echo: write error: Broken pipe
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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> 'wcs_Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits -region wcs_Vir-12-Q2b1x1_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-Q2b1x1_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.qVGbslu81A (6) ############
Parsing command line arguments...
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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> 'wcs_Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_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-Q2b1x1_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(), 5395 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(), 5396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5396 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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits -region wcs_Vir-12-Q2b1x1_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-Q2b1x1_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.58EmTIbgYp (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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=380, passed=5738
Got 5738 stars (including 5354 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat
util/solve_plate_with_UCAC5 got 5738 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.2 to -4.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.2 to -4.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits -region wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.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.5C2GrYfe9m (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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=379, passed=5723
Got 5723 stars (including 5341 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat
util/solve_plate_with_UCAC5 got 5723 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.2 to -4.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.2 to -4.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits -region wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits'
Saving fully-calibrated image wcs_Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits'
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits'
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits'
Preparing the HTML report for the field Vir-12-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20212_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 20212_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:20:01.76 -11:21:40.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Vir-12-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat to cache
SExtractor catalog cache: saved Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Creating symlink local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits exists and is non-empty
wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits exists and is non-empty
wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits exists and is non-empty
wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits (1st reference image)
verification OK: wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Image size: 937.3'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:50.965 -10:00:26.84 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits (1st new image)
verification OK: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
Image size: 937.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:54.357 -09:56:13.90 J2000 4789.000 3195.000
###################################
###################################
# 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 13:42:54.357 -09:56:13.90
Angular distance between the image centers 0.0716 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits (2nd new image)
verification OK: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
Image size: 937.1'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:52.646 -09:56:54.02 J2000 4789.000 3195.000
###################################
###################################
# 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 13:42:52.646 -09:56:54.02
Angular distance between the image centers 0.0595 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 13:42:54.357 -09:56:13.90
Second-epoch second image center 13:42:52.646 -09:56:54.02
Angular distance between the image centers 0.01317 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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits &> /tmp/tmp.I5aM382mlS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits &> /tmp/tmp.rhsgK9BhGg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits &> /tmp/tmp.dJLze4kH08
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits &> /tmp/tmp.iDW2DtbYGL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
Found non-empty wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
The reference image (wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits) and catalog (wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat) found
'wcs_Vir-12-Q2b1x1_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 22.780085
a=0.000000 b=1.000000 c=22.780085
From vast_summary.log: estimated ref. image limiting mag.: -7.80
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.98
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.98
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 40 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
2.3 pix Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
2.4 pix fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
2.4 pix fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
Limiting magnitude estimates:
15.0 mag. Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
15.0 mag. Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
15.0 mag. fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
15.0 mag. fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (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.I5aM382mlS (6) ############
Parsing command line arguments...
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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> 'wcs_Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_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=6, blended=1266, passed=30997
Got 30997 stars (including 29699 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
util/solve_plate_with_UCAC5 got 30997 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 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(), 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: 974 matched stars entering correct_measured_positions(), 30630 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 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(), 30629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 30629 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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits -region wcs_Vir-12-Q2b1x1_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-Q2b1x1_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.rhsgK9BhGg (6) ############
Parsing command line arguments...
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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> 'wcs_Vir-12-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_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=9, blended=1340, passed=30818
Got 30818 stars (including 29441 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat
util/solve_plate_with_UCAC5 got 30818 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(), 30443 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(), 30443 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 30443 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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits -region wcs_Vir-12-Q2b1x1_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-Q2b1x1_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.dJLze4kH08 (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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1735, passed=30991
Got 30991 stars (including 29218 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat
util/solve_plate_with_UCAC5 got 30991 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.2 to -4.5)
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(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 30445 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 429 (Dec -15.2 to -4.5)
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(), 30445 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 30445 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits -region wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.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.iDW2DtbYGL (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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1692, passed=30920
Got 30920 stars (including 29196 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat
util/solve_plate_with_UCAC5 got 30920 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.2 to -4.5)
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(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 30424 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 429 (Dec -15.2 to -4.5)
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(), 30421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 30421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits -region wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.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-Q2b1x1_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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Saving fully-calibrated image wcs_Vir-12-Q2b1x1_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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-28-23_20.00sec_-4.90C_LIGHT_0545.fits
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.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_2026-04-19_CI_Vir-12-Q2b1x1_012950_TTUQ2b1x1_284462_7soDWte8/wcs_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546.fits
Preparing the HTML report for the field Vir-12-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51839.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out51910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52391.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 51837_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 51837_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:43:34.17 -13:17:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51839_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 51839_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:42:32.76 -07:33:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.600 3618571042790708608 205.63641740533 -07.55318811364 14.6734 14.1284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51842_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 51842_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:17:40.44 -05:46:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.981 3634752211819349376 199.41835846023 -05.77830976092 14.5380 14.0141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51910_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
Preparing report for the candidate 51910_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
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Considering the candidate 51922_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
Preparing report for the candidate 51922_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
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Considering the candidate 51929_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
Preparing report for the candidate 51929_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
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Considering the candidate 51959_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
Preparing report for the candidate 51959_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
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Considering the candidate 52009_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52009_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 52158_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52158_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:19:30.15 -11:08:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52174_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52174_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:27:09.57 -11:47:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52213_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52213_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:17:20.66 -12:06:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52238_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52238_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:18:34.71 -12:05:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 1.628 3609634418438699008 199.64500755488 -12.09911542936 14.4843 13.9595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52246_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52246_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:29:22.07 -12:25:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52250_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52250_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:16:47.36 -12:45:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52253_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52253_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:31:13.49 -12:53:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 0.599 3610093601982140928 202.80636340525 -12.89029158061 14.5574 14.0592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52260_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52260_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:18:12.71 -13:01:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.492 3609512613166100608 199.55338362488 -13.02093519752 14.4066 13.8670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52263_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52263_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:22:20.49 -11:40:38.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)
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Considering the candidate 52264_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52264_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:25:38.92 -13:26:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52279_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52279_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:34:32.02 -13:21:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52284_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52284_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:25:47.75 -06:26:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.324 3631513153643042560 201.44889045017 -06.44169051071 14.5409 13.8221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52286_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52286_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:17:38.31 -06:24:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.892 3634505577617189120 199.40945828439 -06.41420270991 14.6403 14.0363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52287_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52287_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:30:41.89 -13:41:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52289_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52289_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:17:52.26 -12:41:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52295_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52295_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:16:35.42 -12:04:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52301_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52301_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:19:27.38 -13:30:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.330 3609193514275838720 199.86417294658 -13.50589092089 14.4618 14.0011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52309_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52309_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:21:33.50 -14:02:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52311_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52311_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:16:05.28 -13:37:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.935 3609361189799058560 199.02249921243 -13.62424082111 14.3697 13.7511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52330_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52330_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:18:50.10 -08:04:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52331_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52331_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:18:46.15 -14:10:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52334_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52334_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:30:28.96 -10:56:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 1.053 3611458954905792640 202.62073596859 -10.95025664502 14.5402 13.9046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52338_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52338_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:17:25.62 -12:33:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.636 3609592052881184256 199.35690291842 -12.55676258204 14.5243 14.0236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52344_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52344_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:20:31.91 -08:48:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 0.538 3624900209677318272 200.13310403594 -08.81431782853 14.5830 13.9799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52345_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52345_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:27:56.00 -11:31:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 1.560 3611412122582233216 201.98369005262 -11.52650619843 14.5802 13.9298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52353_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
Preparing report for the candidate 52353_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
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Considering the candidate 52365_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52365_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:19:52.49 -12:21:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 0.741 3609611358758241664 199.96891074287 -12.35183502889 14.7934 14.0792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52372_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52372_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:20:33.60 -09:56:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.58, MAG_FAINT_SEARCH_LIMIT=15.56)GAIADR2_OUTPUT=# 1.049 3624012457116920704 200.14029392424 -09.94558888583 14.6410 14.1904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52383_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52383_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:35:55.71 -14:03:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52391_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
Preparing report for the candidate 52391_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
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Considering the candidate 52417_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52417_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks
**** FOUND 13:54:50.11 -13:00:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 1.038 3612151544151944832 208.70875484834 -13.01375841420 14.3432 13.5421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52444_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546
The candidate 52444_fd_Vir-12-Q2b1x1_2026-04-19_01-29-12_20.00sec_-4.90C_LIGHT_0546 did not pass the final checks