This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy
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!
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,2461140.8775,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.3775 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461140.8775,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.3775 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461140.8775,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.3775 14.21CV 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 10.3775* 14 04 07.01 +02 24 14.1 13.6 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
V0520 Vir,2461140.8775,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0520 Vir 20260410.3775 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.94661763 22.02.2026 10:42:57.763 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
First image: 2461093.94661763 22.02.2026 10:42:57.763 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Last image: 2461140.87780662 10.04.2026 09:03:52.492 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
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): 5014
Objects passed selection criteria: 5009
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 4671
Average stars matched: 4548.25 (97.3721 %)
Memory usage VmPeak: 111248 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 04:57:06 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.94661763 22.02.2026 10:42:57.763 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
First image: 2461093.94661763 22.02.2026 10:42:57.763 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Last image: 2461140.87780662 10.04.2026 09:03:52.492 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 77
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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): 27164
Objects passed selection criteria: 27096
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 24701.8
Average stars matched: 23826.5 (96.4567 %)
Memory usage VmPeak: 131072 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 04:57:59 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
SExtractor catalog cache: saved Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat to cache
SExtractor catalog cache: saved Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.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: 2461140.87728333
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits exists and is non-empty
Saving wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits to local_wcs_cache/
'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits' -> 'local_wcs_cache/wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits'
wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits exists and is non-empty
Saving wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits to local_wcs_cache/
'wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits' -> 'local_wcs_cache/wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits'
wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits exists and is non-empty
Saving wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits to local_wcs_cache/
'wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits' -> 'local_wcs_cache/wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits'
wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits exists and is non-empty
Saving wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits to local_wcs_cache/
'wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits' -> 'local_wcs_cache/wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:42:51.358 +05:59:16.47
Second-epoch image center 13:42:41.918 +06:03:33.42
Angular distance between the image centers 0.0814 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:42:51.358 +05:59:16.47
Second-epoch image center 13:42:42.587 +06:03:33.45
Angular distance between the image centers 0.0801 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:42:41.918 +06:03:33.42
Second-epoch second image center 13:42:42.587 +06:03:33.45
Angular distance between the image centers 0.00277 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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits &> /tmp/tmp.WsLrJth3kG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits &> /tmp/tmp.NjUsNIW7PD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits &> /tmp/tmp.cdk0YjjMCI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits &> /tmp/tmp.xqtgjaGM7F
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
Found non-empty wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
The reference image (wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits) and catalog (wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat) found
'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat' -> 'wcsmag.cat'
Read 6371 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6203 to 214.0565 deg, Dec +0.1313 to +11.7245 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 197.6203 to 214.0565 deg, Dec 0.1313 to 11.7245 deg
Loaded 4511 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): 3361 out of 3468 total matches.
Matched with Tycho-2 3468 out of 6371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.948201
a=0.000000 b=1.000000 c=22.948201
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
2.3 pix Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
2.8 pix fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
2.8 pix fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
Limiting magnitude estimates:
15.3 mag. Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
15.3 mag. Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
15.0 mag. fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
15.0 mag. fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.2 (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.WsLrJth3kG (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits' -> 'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS_IMAGE_NAME=wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS-calibrated image found: wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Checking if the catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits alredy exist and is non-empty...
Catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS catalog name: wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=356, passed=6371
Got 6371 stars (including 6012 good ones) from the SExtractor catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
util/solve_plate_with_UCAC5 got 6371 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits -region wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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.NjUsNIW7PD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits' -> 'wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS_IMAGE_NAME=wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS-calibrated image found: wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Checking if the catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits alredy exist and is non-empty...
Catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS catalog name: wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=378, passed=6255
Got 6255 stars (including 5875 good ones) from the SExtractor catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat
util/solve_plate_with_UCAC5 got 6255 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6164 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits -region wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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.cdk0YjjMCI (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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
WCS_IMAGE_NAME=wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
WCS-calibrated image found: wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
Checking if the catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
WCS catalog name: wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=574, passed=5565
Got 5565 stars (including 4987 good ones) from the SExtractor catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat
util/solve_plate_with_UCAC5 got 5565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits -region wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.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.xqtgjaGM7F (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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
WCS_IMAGE_NAME=wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
WCS-calibrated image found: wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
Checking if the catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
WCS catalog name: wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=565, passed=5541
Got 5541 stars (including 4972 good ones) from the SExtractor catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat
util/solve_plate_with_UCAC5 got 5541 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (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 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits -region wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits'
Saving fully-calibrated image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits'
Saving fully-calibrated image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits'
Saving fully-calibrated image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits'
Preparing the HTML report for the field Vir-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Vir-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
SExtractor catalog cache: saved Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat to cache
SExtractor catalog cache: saved Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Creating symlink local_wcs_cache/wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits exists and is non-empty
wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits exists and is non-empty
wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits exists and is non-empty
wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:42:51.358 +05:59:16.47
Second-epoch image center 13:42:41.918 +06:03:33.42
Angular distance between the image centers 0.0814 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:42:51.358 +05:59:16.47
Second-epoch image center 13:42:42.587 +06:03:33.45
Angular distance between the image centers 0.0801 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:42:41.918 +06:03:33.42
Second-epoch second image center 13:42:42.587 +06:03:33.45
Angular distance between the image centers 0.00277 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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits &> /tmp/tmp.DmzYrPiCeu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits &> /tmp/tmp.PA0QE7PN6d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits &> /tmp/tmp.HmBYMmNmDP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits &> /tmp/tmp.u7NMIfjpT4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
Found non-empty wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
The reference image (wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits) and catalog (wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat) found
'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat' -> 'wcsmag.cat'
Read 33426 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.5473 to 214.0698 deg, Dec +0.1166 to +11.7520 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 197.5473 to 214.0698 deg, Dec 0.1166 to 11.7520 deg
Loaded 4535 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): 3241 out of 3477 total matches.
Matched with Tycho-2 3477 out of 33426 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.827622
a=0.000000 b=1.000000 c=22.827622
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
2.2 pix Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
2.6 pix fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
2.6 pix fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
Limiting magnitude estimates:
15.5 mag. Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
15.5 mag. Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
15.1 mag. fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
15.2 mag. fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.5 (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.DmzYrPiCeu (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits' -> 'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS_IMAGE_NAME=wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS-calibrated image found: wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Checking if the catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits alredy exist and is non-empty...
Catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS catalog name: wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1360, passed=33416
Got 33416 stars (including 32008 good ones) from the SExtractor catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
util/solve_plate_with_UCAC5 got 33416 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 33035 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 33036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 33036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits -region wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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.PA0QE7PN6d (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits' -> 'wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS_IMAGE_NAME=wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS-calibrated image found: wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Checking if the catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits alredy exist and is non-empty...
Catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS catalog name: wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1371, passed=33591
Got 33591 stars (including 32174 good ones) from the SExtractor catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat
util/solve_plate_with_UCAC5 got 33591 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 33126 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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 33125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 33125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits -region wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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.HmBYMmNmDP (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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
WCS_IMAGE_NAME=wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
WCS-calibrated image found: wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
Checking if the catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
WCS catalog name: wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=2177, passed=26020
Got 26020 stars (including 23817 good ones) from the SExtractor catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat
util/solve_plate_with_UCAC5 got 26020 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 25058 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 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 25058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 25058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits -region wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.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.u7NMIfjpT4 (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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
WCS_IMAGE_NAME=wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
WCS-calibrated image found: wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
Checking if the catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
WCS catalog name: wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2187, passed=26021
Got 26021 stars (including 23807 good ones) from the SExtractor catalog wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat
util/solve_plate_with_UCAC5 got 26021 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (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 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 25083 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 453 to 508 (Dec 0.7 to 11.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 25082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 25080 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits -region wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Saving fully-calibrated image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Saving fully-calibrated image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-07_20.00sec_-4.90C_LIGHT_0270.fits
Saving fully-calibrated image wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.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_2026-04-10_CI_Vir-04-Q2b1x1_044928_TTUQ2b1x1_1318_C26HNiCy/wcs_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271.fits
Preparing the HTML report for the field Vir-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out28528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52810.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 52049_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52049_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:57:26.23 +04:48:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 1.072 3671891756100323456 209.35916667666 +04.80367390013 14.4625 13.8349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52053_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52053_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:25:48.33 +09:01:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52054_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52054_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:00:09.45 +03:55:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52148_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52148_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 52167_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52167_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 52176_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52176_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 52237_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52237_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 52268_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52268_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52285_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
Preparing report for the candidate 52285_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
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Considering the candidate 52301_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52301_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 52343_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52343_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:07:51.99 +02:46:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52456_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52456_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:00:28.37 +07:02:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52481_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52481_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:04:19.45 +02:35:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52484_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52484_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:31:29.11 +04:16:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52519_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52519_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:33:52.88 +03:09:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52535_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52535_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:49:38.59 +08:23:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52573_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
Preparing report for the candidate 52573_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
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Considering the candidate 52583_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52583_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 52635_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52635_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:38:46.75 +09:57:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52650_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52650_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52654_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52654_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52674_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52674_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 52743_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52743_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:02:41.49 +02:14:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 0.339 3664419883099255936 210.67280620283 +02.23782433772 14.6415 14.1008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52751_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52751_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:02:08.17 +02:19:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52775_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52775_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:08:07.33 +02:36:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 0.424 3667406298414776448 212.03062608474 +02.60627908893 14.5791 13.9087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52778_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52778_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:00:27.01 +07:02:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52810_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
Preparing report for the candidate 52810_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
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Considering the candidate 52811_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52811_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:49:58.25 +09:39:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.707 3725286823883873920 207.49245255929 +09.65642927671 14.2861 13.6350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52841_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52841_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:00:05.41 +02:00:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 1.835 3664400714660746496 210.02203679519 +02.00107299201 14.8635 14.6736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52855_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52855_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 52864_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52864_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:53:24.33 +09:06:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 2.279 3722151429038417792 208.35109630793 +09.10929098573 14.2906 13.3753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52905_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52905_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:06:24.42 +03:08:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52907_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52907_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:10:03.80 +02:28:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 0.700 3667292945637814656 212.51571050084 +02.47465075316 14.7487 14.1785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52910_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52910_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:57:49.77 +04:20:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.786 3671671235299458688 209.45732594116 +04.34550635337 14.6682 14.0933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52923_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52923_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:06:26.50 +04:16:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.572 3671279671720903040 211.61003172680 +04.26923610601 14.8748 14.6117 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52930_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52930_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:03:57.33 +02:36:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.001 3670441053586590464 210.98894519410 +02.60945310789 14.3218 13.2382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52935_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52935_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:57:05.75 +03:24:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 2.231 3665545718582154240 209.27339782117 +03.41440004674 14.8606 14.2571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52939_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52939_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 52944_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52944_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:52:22.83 +02:20:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52958_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52958_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52963_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52963_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:06:37.41 +03:58:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 2.637 3670707307199311232 211.65598900259 +03.96638763030 14.8901 14.1738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52972_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52972_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:02:15.51 +05:12:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 1.008 3672194946431616256 210.56445885708 +05.20321848234 14.4690 13.4339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52982_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52982_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:03:40.34 +08:44:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52990_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 52990_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:44:09.65 +05:22:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 3.181 3714296827207042176 206.03977680802 +05.37928347632 15.0812 14.5383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53000_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 53000_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:49:39.05 +04:15:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.808 3713922855814682624 207.41220613265 +04.25301093244 15.0153 14.3642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53006_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 53006_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:01:30.90 +03:01:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.550 3670528602199930368 210.37842513945 +03.02061659198 15.1479 14.6476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53007_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 53007_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:04:24.49 +02:21:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 0.615 3667427395294031232 211.10187477736 +02.35007434614 14.6244 14.0678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53028_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 53028_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 14:02:10.31 +08:11:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 0.339 3722543370573862144 210.54294769958 +08.18964914671 14.4105 13.2914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53045_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 53045_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
**** FOUND 13:59:11.62 +08:23:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 2.289 3722598380514921344 209.79779349795 +08.39120563834 15.3732 15.0513 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53109_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 53109_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 53160_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271
The candidate 53160_fd_Vir-04-Q2b1x1_2026-04-10_04-03-52_20.00sec_-4.90C_LIGHT_0271 did not pass the final checks