This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4517* 14 04 21.48 -04 40 31.7 10.2 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.9516,10.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4516 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4517* 14 19 07.81 +00 30 28.8 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,2461143.9516,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.4516 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4517* 14 23 57.79 -01 00 08.9 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
ASAS J142357-0100.1,2461143.9516,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J142357-0100.1 20260413.4516 12.62CV 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: 2461098.89777297 27.02.2026 09:32:37.585 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
First image: 2461098.89777297 27.02.2026 09:32:37.585 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
Last image: 2461143.95202568 13.04.2026 10:50:45.019 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.10
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5573
Objects passed selection criteria: 5559
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 4259
Average stars matched: 3827.25 (89.8626 %)
Memory usage VmPeak: 111932 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 05:52:47 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.89777297 27.02.2026 09:32:37.585 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
First image: 2461098.89777297 27.02.2026 09:32:37.585 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
Last image: 2461143.95202568 13.04.2026 10:50:45.019 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.82
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: 13 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): 31119
Objects passed selection criteria: 31041
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 24468.5
Average stars matched: 22102.2 (90.3294 %)
Memory usage VmPeak: 135812 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 05:53:40 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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
SExtractor catalog cache: saved Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat to cache
SExtractor catalog cache: saved Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461143.95126797
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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits exists and is non-empty
Saving wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits to local_wcs_cache/
'wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits' -> 'local_wcs_cache/wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits'
wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits exists and is non-empty
Saving wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits to local_wcs_cache/
'wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits' -> 'local_wcs_cache/wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits'
wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits exists and is non-empty
Saving wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits to local_wcs_cache/
'wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits' -> 'local_wcs_cache/wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits'
wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits exists and is non-empty
Saving wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits to local_wcs_cache/
'wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits' -> 'local_wcs_cache/wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:34:14.524 -01:59:52.47
Second-epoch image center 14:34:07.190 -02:02:33.48
Angular distance between the image centers 0.0542 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:14.524 -01:59:52.47
Second-epoch image center 14:34:04.677 -02:02:15.81
Angular distance between the image centers 0.0572 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 14:34:07.190 -02:02:33.48
Second-epoch second image center 14:34:04.677 -02:02:15.81
Angular distance between the image centers 0.01156 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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits &> /tmp/tmp.1KRlRX4gNK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits &> /tmp/tmp.Lvo1SgPfWM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits &> /tmp/tmp.KsXjuz7od0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits &> /tmp/tmp.I6JxmKkhpn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits and wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits and wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat
Found non-empty wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits and wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat
The reference image (wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits) and catalog (wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat) found
'wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat' -> 'wcsmag.cat'
Read 5573 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.6462 to 226.4343 deg, Dec -7.2848 to +3.3063 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 210.6462 to 226.4343 deg, Dec -7.2848 to 3.3063 deg
Loaded 3983 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): 3276 out of 3378 total matches.
Matched with Tycho-2 3378 out of 5573 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.937037
a=0.000000 b=1.000000 c=22.937037
From vast_summary.log: estimated ref. image limiting mag.: -8.10
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.84
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
2.4 pix Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
2.5 pix fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
2.5 pix fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
Limiting magnitude estimates:
14.8 mag. Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
15.2 mag. Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
13.0 mag. fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
13.2 mag. fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.1KRlRX4gNK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits' -> 'wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
WCS_IMAGE_NAME=wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
WCS-calibrated image found: wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
Checking if the catalog wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits alredy exist and is non-empty...
Catalog wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
WCS catalog name: wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=359, passed=5573
Got 5573 stars (including 5212 good ones) from the SExtractor catalog wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat
util/solve_plate_with_UCAC5 got 5573 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 5459 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 5461 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 5461 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits -region wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Lvo1SgPfWM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.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-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits' -> 'wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
Checking if the catalog wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
WCS catalog name: wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=435, passed=7095
Got 7095 stars (including 6657 good ones) from the SExtractor catalog wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat
util/solve_plate_with_UCAC5 got 7095 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6938 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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits -region wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.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.KsXjuz7od0 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
WCS_IMAGE_NAME=wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
WCS-calibrated image found: wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
Checking if the catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
WCS catalog name: wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=78, passed=2137
Got 2137 stars (including 2056 good ones) from the SExtractor catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat
util/solve_plate_with_UCAC5 got 2137 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 411 to 469 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 2096 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 411 to 469 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 2098 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 2098 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 918 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits -region wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.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.I6JxmKkhpn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
WCS_IMAGE_NAME=wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
WCS-calibrated image found: wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
Checking if the catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
WCS catalog name: wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=226, passed=2379
Got 2379 stars (including 2148 good ones) from the SExtractor catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat
util/solve_plate_with_UCAC5 got 2379 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 411 to 469 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 2342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 411 to 469 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 2341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 2341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 929 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits -region wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits'
Saving fully-calibrated image wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits'
Saving fully-calibrated image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits'
Saving fully-calibrated image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits'
Preparing the HTML report for the field Vir-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out21575.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 21575_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
Preparing report for the candidate 21575_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
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-09-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 ####
14:04:21.48 -04:40:31.7
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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
SExtractor catalog cache: saved Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat to cache
SExtractor catalog cache: saved Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
Creating symlink local_wcs_cache/wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits exists and is non-empty
wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits exists and is non-empty
wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits exists and is non-empty
wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:34:14.524 -01:59:52.47
Second-epoch image center 14:34:07.190 -02:02:33.48
Angular distance between the image centers 0.0542 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:14.524 -01:59:52.47
Second-epoch image center 14:34:04.677 -02:02:15.81
Angular distance between the image centers 0.0572 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 14:34:07.190 -02:02:33.48
Second-epoch second image center 14:34:04.677 -02:02:15.81
Angular distance between the image centers 0.01156 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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits &> /tmp/tmp.K9WxW3UDFL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits &> /tmp/tmp.3U4rzTN0ww
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits &> /tmp/tmp.ha6LgdEmm2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits &> /tmp/tmp.WsEkNQ0CEh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits and wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits and wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat
Found non-empty wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits and wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat
The reference image (wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits) and catalog (wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat) found
'wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat' -> 'wcsmag.cat'
Read 31995 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 210.6462 to 226.4399 deg, Dec -7.2858 to +3.3064 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 210.6462 to 226.4399 deg, Dec -7.2858 to 3.3064 deg
Loaded 3985 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): 3266 out of 3501 total matches.
Matched with Tycho-2 3501 out of 31995 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.802511
a=0.000000 b=1.000000 c=22.802511
From vast_summary.log: estimated ref. image limiting mag.: -7.82
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.98
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.98
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
2.3 pix Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
2.5 pix fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
2.5 pix fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
Limiting magnitude estimates:
15.0 mag. Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
15.3 mag. Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
13.3 mag. fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
13.4 mag. fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 13.0 (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.K9WxW3UDFL (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits' -> 'wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
WCS_IMAGE_NAME=wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
WCS-calibrated image found: wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
Checking if the catalog wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits alredy exist and is non-empty...
Catalog wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
WCS catalog name: wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1383, passed=31983
Got 31983 stars (including 30562 good ones) from the SExtractor catalog wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat
util/solve_plate_with_UCAC5 got 31983 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 31204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 31205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 31205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits -region wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3U4rzTN0ww (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.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-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits' -> 'wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
Checking if the catalog wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
WCS catalog name: wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1924, passed=40006
Got 40006 stars (including 38039 good ones) from the SExtractor catalog wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat
util/solve_plate_with_UCAC5 got 40006 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 38759 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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 38758 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 38758 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits -region wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.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.ha6LgdEmm2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
WCS_IMAGE_NAME=wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
WCS-calibrated image found: wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
Checking if the catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
WCS catalog name: wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=299, passed=13190
Got 13190 stars (including 12870 good ones) from the SExtractor catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat
util/solve_plate_with_UCAC5 got 13190 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 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 12913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 12913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 12913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 920 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits -region wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.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.WsEkNQ0CEh (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
WCS_IMAGE_NAME=wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
WCS-calibrated image found: wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
Checking if the catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
WCS catalog name: wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=340, passed=13668
Got 13668 stars (including 13306 good ones) from the SExtractor catalog wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat
util/solve_plate_with_UCAC5 got 13668 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 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 13435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 13433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 13433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits -region wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.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-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/wcs_Vir-09-Q1b1x1_2026-02-27_03-32-37_20.00sec_-15.00C_LIGHT_0189.fits
Saving fully-calibrated image wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/wcs_Vir-09-Q1b1x1_2026-03-20_03-41-36_20.00sec_-15.00C_LIGHT_0401.fits
Saving fully-calibrated image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-49-39_20.00sec_-4.90C_LIGHTs_0219.fits
Saving fully-calibrated image wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vir-09-Q1b1x1_055144_TTUQ1b1x1_14747_uq3EWG51/wcs_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220.fits
Preparing the HTML report for the field Vir-09-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out00990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out01387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out02048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out02424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out02642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out05581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out59019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out59105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out18536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59207.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 58919_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
The candidate 58919_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220 did not pass the final checks
**** FOUND 14:04:21.48 -04:40:31.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 59019_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
The candidate 59019_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220 did not pass the final checks
**** FOUND 14:47:51.24 -05:48:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 1.328 6336910987513309568 221.96313276768 -05.80117220079 12.1095 11.5514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 59105_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
The candidate 59105_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220 did not pass the final checks
**** FOUND 14:45:31.29 -06:55:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.494 6330638617274711296 221.38077905502 -06.92244031744 12.5874 12.0538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 59207_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
Preparing report for the candidate 59207_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
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Considering the candidate 02424_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
The candidate 02424_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220 did not pass the final checks
**** FOUND 14:58:57.25 -06:19:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.414 6333877572371479040 224.73844737356 -06.32573354485 12.1852 11.5937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 18536_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
Preparing report for the candidate 18536_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
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Considering the candidate 05581_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
The candidate 05581_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220 did not pass the final checks
**** FOUND 15:03:15.78 -05:15:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.200 6335722690321590528 225.81577907417 -05.25167484601 12.1460 11.6437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 02048_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
The candidate 02048_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220 did not pass the final checks
**** FOUND 15:01:16.15 -06:27:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.988 6333813495755281920 225.31701824114 -06.46259975841 12.4222 11.7441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 02642_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
The candidate 02642_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220 did not pass the final checks
**** FOUND 15:01:45.14 -06:15:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.043 6333914410306935680 225.43788208015 -06.25704037202 12.7716 12.2455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 01387_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
The candidate 01387_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220 did not pass the final checks
**** FOUND 15:02:18.67 -06:44:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.438 6333043150421259008 225.57767972105 -06.73524409830 12.3183 11.7770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 03881_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
The candidate 03881_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220 did not pass the final checks
**** FOUND 14:42:00.60 -05:49:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 00990_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220
The candidate 00990_fd_Vir-09-Q1b1x1_2026-04-13_05-50-45_20.00sec_-4.90C_LIGHTs_0220 did not pass the final checks