This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo
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 18.3842* 13 46 36.80 -17 37 20.9 10.8 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461148.8841,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260418.3841 10.83CV 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 18.3842* 13 40 40.28 -13 24 41.7 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,2461148.8841,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260418.3841 11.96CV 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 18.3842* 13 19 55.90 -21 10 32.8 12.6 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461148.8841,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260418.3841 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 18.3842* 13 52 29.29 -17 30 39.7 13.3 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461148.8841,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260418.3841 13.28CV 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 18.3842* 13 08 48.97 -20 45 48.1 13.7 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,2461148.8841,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260418.3841 13.65CV 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: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
First image: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Last image: 2461148.88454117 18.04.2026 09:13:34.357 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.18
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: 2 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): 5180
Objects passed selection criteria: 5177
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 4791.5
Average stars matched: 4638.25 (96.8016 %)
Memory usage VmPeak: 110996 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 Sat Apr 18 05:04:10 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
First image: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Last image: 2461148.88454117 18.04.2026 09:13:34.357 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 45
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.89
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): 33586
Objects passed selection criteria: 33521
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 31421
Average stars matched: 30058 (95.6621 %)
Memory usage VmPeak: 134064 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 Sat Apr 18 05:05:07 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
SExtractor catalog cache: saved Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat to cache
SExtractor catalog cache: saved Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.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: 2461148.88375654
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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits exists and is non-empty
Saving wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits to local_wcs_cache/
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> 'local_wcs_cache/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits exists and is non-empty
Saving wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits to local_wcs_cache/
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> 'local_wcs_cache/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits exists and is non-empty
Saving wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits to local_wcs_cache/
'wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits' -> 'local_wcs_cache/wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits'
wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits exists and is non-empty
Saving wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits to local_wcs_cache/
'wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits' -> 'local_wcs_cache/wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits (1st reference image)
verification OK: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Image size: 941.6'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:20:00.735 -18:00:04.53 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits (1st new image)
verification OK: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
Image size: 941.8'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:19:56.913 -17:59:31.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:19:56.913 -17:59:31.46
Angular distance between the image centers 0.0177 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits (2nd new image)
verification OK: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
Image size: 941.8'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:19:54.381 -17:59:05.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:19:54.381 -17:59:05.49
Angular distance between the image centers 0.0301 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 13:19:56.913 -17:59:31.46
Second-epoch second image center 13:19:54.381 -17:59:05.49
Angular distance between the image centers 0.01236 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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits &> /tmp/tmp.V5vBKND3PM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits &> /tmp/tmp.Zw4cOmHBXy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits &> /tmp/tmp.yiScAwQ92K
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits &> /tmp/tmp.qdeiJo3SMF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
Found non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
The reference image (wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits) and catalog (wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat) found
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat' -> 'wcsmag.cat'
Read 5029 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 191.6471 to 208.5697 deg, Dec -23.3251 to -12.4821 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 191.6471 to 208.5697 deg, Dec -23.3251 to -12.4821 deg
Loaded 5144 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): 3620 out of 3751 total matches.
Matched with Tycho-2 3751 out of 5029 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.824361
a=0.000000 b=1.000000 c=22.824361
From vast_summary.log: estimated ref. image limiting mag.: -8.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.64
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.64
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
2.1 pix Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
2.3 pix fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
2.3 pix fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
Limiting magnitude estimates:
14.6 mag. Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
14.6 mag. Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
14.5 mag. fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
14.5 mag. fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.6 (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.V5vBKND3PM (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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> 'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Checking if the catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS catalog name: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=403, passed=5029
Got 5029 stars (including 4621 good ones) from the SExtractor catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 5029 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
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(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
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(), 4964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits -region wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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.Zw4cOmHBXy (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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> 'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS-calibrated image found: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Checking if the catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS catalog name: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=395, passed=5063
Got 5063 stars (including 4663 good ones) from the SExtractor catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
util/solve_plate_with_UCAC5 got 5063 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
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(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
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(), 5001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits -region wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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.yiScAwQ92K (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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
Checking if the catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
WCS catalog name: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=297, passed=4597
Got 4597 stars (including 4293 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat
util/solve_plate_with_UCAC5 got 4597 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4545 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4545 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4545 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits -region wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.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.qdeiJo3SMF (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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
Checking if the catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
WCS catalog name: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=299, passed=4603
Got 4603 stars (including 4297 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat
util/solve_plate_with_UCAC5 got 4603 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 390 (Dec -23.6 to -12.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 390 (Dec -23.6 to -12.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits -region wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
Saving fully-calibrated image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
Saving fully-calibrated image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits'
Saving fully-calibrated image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits'
Preparing the HTML report for the field Vir-13-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20342.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20342_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
Preparing report for the candidate 20342_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20441_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 20441_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:16:01.83 -17:14:51.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20464_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 20464_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:32:13.32 -19:39:50.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02207_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 02207_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:00:41.26 -17:38:47.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Vir-13-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:46:36.80 -17:37:20.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
SExtractor catalog cache: saved Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat to cache
SExtractor catalog cache: saved Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Creating symlink local_wcs_cache/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits exists and is non-empty
wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits exists and is non-empty
wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits exists and is non-empty
wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits (1st reference image)
verification OK: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Image size: 941.6'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:20:00.735 -18:00:04.53 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits (1st new image)
verification OK: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
Image size: 941.8'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:19:56.913 -17:59:31.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:19:56.913 -17:59:31.46
Angular distance between the image centers 0.0177 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits (2nd new image)
verification OK: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
Image size: 941.8'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:19:54.381 -17:59:05.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:19:54.381 -17:59:05.49
Angular distance between the image centers 0.0301 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 13:19:56.913 -17:59:31.46
Second-epoch second image center 13:19:54.381 -17:59:05.49
Angular distance between the image centers 0.01236 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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits &> /tmp/tmp.Hyjz13HTk7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits &> /tmp/tmp.Ih3nkrFgft
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits &> /tmp/tmp.OXNNc3IzYA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits &> /tmp/tmp.hKrDzNnOm4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
Found non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
The reference image (wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits) and catalog (wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat) found
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat' -> 'wcsmag.cat'
Read 33033 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 191.6273 to 208.6562 deg, Dec -23.3283 to -12.4172 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 191.6273 to 208.6562 deg, Dec -23.3283 to -12.4172 deg
Loaded 5201 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): 4068 out of 4378 total matches.
Matched with Tycho-2 4378 out of 33033 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.651881
a=0.000000 b=1.000000 c=22.651881
From vast_summary.log: estimated ref. image limiting mag.: -7.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.76
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
2.1 pix Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
2.2 pix fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
2.2 pix fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
Limiting magnitude estimates:
14.8 mag. Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
14.8 mag. Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
14.6 mag. fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
14.6 mag. fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (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.Hyjz13HTk7 (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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> 'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Checking if the catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS catalog name: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1226, passed=33024
Got 33024 stars (including 31738 good ones) from the SExtractor catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 33024 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits -region wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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.Ih3nkrFgft (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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> 'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS-calibrated image found: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Checking if the catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS catalog name: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1202, passed=32716
Got 32716 stars (including 31457 good ones) from the SExtractor catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
util/solve_plate_with_UCAC5 got 32716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32336 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32336 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32336 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits -region wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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.OXNNc3IzYA (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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
Checking if the catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
WCS catalog name: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1030, passed=30461
Got 30461 stars (including 29388 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat
util/solve_plate_with_UCAC5 got 30461 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 30124 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 30124 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 30124 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits -region wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.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.hKrDzNnOm4 (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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
Checking if the catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
WCS catalog name: wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1095, passed=30506
Got 30506 stars (including 29356 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat
util/solve_plate_with_UCAC5 got 30506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
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(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 30125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
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(), 30125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 30125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits -region wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.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-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Saving fully-calibrated image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Saving fully-calibrated image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-12-26_20.00sec_-4.90C_LIGHTs_0125.fits
Saving fully-calibrated image wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.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_2026-04-18_CI_Vir-13-Q1b1x1_041433_TTUQ1b1x1_2863257_DsEc1CVo/wcs_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126.fits
Preparing the HTML report for the field Vir-13-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52385.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53350.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52383_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52383_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:16:05.08 -16:54:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.163 3511365772864605952 199.02118954743 -16.90462708895 14.4278 13.7622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52385_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52385_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:20:06.14 -17:07:05.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52388_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52388_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:21:37.84 -16:17:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52389_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52389_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:23:45.06 -14:57:52.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 52390_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52390_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:24:08.29 -15:50:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52391_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52391_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:23:10.24 -15:14:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.915 3608020369728761600 200.79216273341 -15.23354893780 14.0500 13.5227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52392_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52392_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:50:39.44 -13:00:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.848 3529141508631338496 192.66480219510 -13.00812280844 13.3959 12.9695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52394_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52394_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:22:42.08 -15:35:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52472_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52472_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:46:36.80 -17:37:20.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52611_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52611_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:50:18.08 -12:48:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52631_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
Preparing report for the candidate 52631_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
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Considering the candidate 52828_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
Preparing report for the candidate 52828_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
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Considering the candidate 52841_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 52841_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:58:48.81 -15:07:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53176_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
Preparing report for the candidate 53176_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
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Considering the candidate 53182_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53182_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:14:08.53 -12:45:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53350_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
Preparing report for the candidate 53350_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
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Considering the candidate 53389_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53389_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:05:50.32 -12:55:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53475_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53475_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:46:43.82 -20:20:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53502_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53502_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:51:50.08 -22:34:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53541_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53541_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:41:39.16 -22:53:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53553_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53553_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:54:38.76 -16:10:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53563_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53563_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:48:13.65 -21:31:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53672_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53672_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:05:05.53 -12:47:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53756_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53756_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:13:08.80 -22:48:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 0.780 3504396484052144768 198.28690050784 -22.81028342034 14.1750 13.5696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53758_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53758_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:55:44.16 -13:00:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.595 3526196123138982912 193.93395239069 -13.01601982385 14.2982 13.8227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53759_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53759_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:43:40.08 -22:59:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53783_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53783_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:33:51.37 -22:41:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53788_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53788_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:23:19.80 -14:53:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53792_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53792_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:13:22.12 -20:41:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.041 3506428141022005120 198.34203715921 -20.69943198411 13.9873 12.9380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53800_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53800_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:24:15.06 -18:20:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53812_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53812_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:00:34.83 -13:14:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 0.690 3525946156042417408 195.14531558551 -13.23685412199 14.3208 13.8500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53813_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53813_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:52:42.42 -18:27:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.351 3510299143506451200 193.17713625963 -18.45550250989 14.5534 14.1549 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53825_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53825_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:52:17.04 -15:53:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53874_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53874_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:13:48.44 -21:51:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.315 3504788597386312704 198.45221686996 -21.86514670035 14.5402 14.0277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53881_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53881_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:00:18.17 -13:18:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53902_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53902_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:50:01.23 -16:00:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 0.279 3522926897112512128 192.50504460489 -16.01130096802 14.1525 13.5507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53922_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53922_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:16:19.73 -22:18:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 0.242 3504519251397284864 199.08228072643 -22.30496733022 14.2458 13.5587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53925_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53925_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:31:23.71 -22:34:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.842 6195186726127747840 202.84933377286 -22.57491126553 14.4638 14.2793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53937_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53937_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:01:46.78 -20:51:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 0.055 3505487543184249600 195.44491060469 -20.85004183040 14.2102 13.5561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53941_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 53941_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 12:51:33.86 -20:16:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 2.737 3509470833293648384 192.89155307280 -20.27784170794 14.3780 13.9032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 14492_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 14492_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks
**** FOUND 13:00:41.26 -17:38:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32176_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126
The candidate 32176_fd_Vir-13-Q1b1x1_2026-04-18_04-13-34_20.00sec_-4.90C_LIGHTs_0126 did not pass the final checks