This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2833* 13 16 57.54 -10 12 46.2 11.9 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7833,11.93,0.05,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 20260409.2833 11.93CV 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 09.2833* 13 25 26.24 -13 10 24.5 12.1 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7833,12.05,0.05,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 20260409.2833 12.05CV 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 09.2833* 13 37 03.18 -08 28 06.8 12.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7833,12.43,0.05,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 20260409.2833 12.43CV 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 09.2833* 13 20 06.95 -06 07 19.8 14.2 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7833,14.16,0.05,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 20260409.2833 14.16CV 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 09.2833* 13 46 39.12 -10 41 21.2 14.3 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7833,14.35,0.05,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 20260409.2833 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.90743030 27.02.2026 09:46:31.978 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
First image: 2461098.90743030 27.02.2026 09:46:31.978 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Last image: 2461139.78356010 09.04.2026 06:48:09.593 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.09
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 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): 4611
Objects passed selection criteria: 4610
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 4398.5
Average stars matched: 4185.75 (95.1631 %)
Memory usage VmPeak: 110992 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 Thu Apr 9 02:17:47 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.90743030 27.02.2026 09:46:31.978 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
First image: 2461098.90743030 27.02.2026 09:46:31.978 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Last image: 2461139.78356010 09.04.2026 06:48:09.593 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 87
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.80
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 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): 25595
Objects passed selection criteria: 25560
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 24566.5
Average stars matched: 23597.5 (96.0556 %)
Memory usage VmPeak: 129484 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 Thu Apr 9 02:18:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat to cache
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.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: 2461139.78301572
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits exists and is non-empty
Saving wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits to local_wcs_cache/
'wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> 'local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits'
wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits exists and is non-empty
Saving wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits to local_wcs_cache/
'wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> 'local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits'
wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits exists and is non-empty
Saving wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits to local_wcs_cache/
'wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits' -> 'local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits'
wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits exists and is non-empty
Saving wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits to local_wcs_cache/
'wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits' -> 'local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:42:50.965 -10:00:26.84
Second-epoch image center 13:42:54.071 -09:58:14.56
Angular distance between the image centers 0.0389 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:42:50.965 -10:00:26.84
Second-epoch image center 13:42:56.340 -09:58:28.47
Angular distance between the image centers 0.0396 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:42:54.071 -09:58:14.56
Second-epoch second image center 13:42:56.340 -09:58:28.47
Angular distance between the image centers 0.01008 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits &> /tmp/tmp.8kYRXGHQ6a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits &> /tmp/tmp.NKAaGnl9yg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits &> /tmp/tmp.LFvydkHTe0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits &> /tmp/tmp.2mosRIqdDX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
Found non-empty wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
The reference image (wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits) and catalog (wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat) found
'wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat' -> 'wcsmag.cat'
Read 5441 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6102 to 213.7377 deg, Dec -15.2798 to -4.6610 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 197.6102 to 213.7377 deg, Dec -15.2798 to -4.6610 deg
Loaded 4386 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3481 out of 3580 total matches.
Matched with Tycho-2 3580 out of 5441 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.918872
a=0.000000 b=1.000000 c=22.918872
From vast_summary.log: estimated ref. image limiting mag.: -8.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.83
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.83
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
2.4 pix Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
3.1 pix fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
3.0 pix fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
Limiting magnitude estimates:
14.8 mag. Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
14.8 mag. Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
14.8 mag. fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
14.8 mag. fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.8kYRXGHQ6a (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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> 'wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=359, passed=5441
Got 5441 stars (including 5082 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
util/solve_plate_with_UCAC5 got 5441 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits -region wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NKAaGnl9yg (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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> 'wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=377, passed=5451
Got 5451 stars (including 5071 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat
util/solve_plate_with_UCAC5 got 5451 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5395 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits -region wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LFvydkHTe0 (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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=412, passed=5967
Got 5967 stars (including 5555 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat
util/solve_plate_with_UCAC5 got 5967 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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits -region wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.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.2mosRIqdDX (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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=422, passed=6020
Got 6020 stars (including 5596 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat
util/solve_plate_with_UCAC5 got 6020 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits -region wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits'
Saving fully-calibrated image wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits'
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits'
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits'
Preparing the HTML report for the field Vir-12-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20207.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20204_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 20204_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:20:01.78 -11:21:41.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20206_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 20206_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:35:17.80 -10:28:37.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20207_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
Preparing report for the candidate 20207_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20213_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 20213_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:22:24.80 -07:32:35.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Vir-12-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:16:57.54 -10:12:46.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat to cache
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Creating symlink local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits exists and is non-empty
wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits exists and is non-empty
wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits exists and is non-empty
wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:42:50.965 -10:00:26.84
Second-epoch image center 13:42:54.071 -09:58:14.56
Angular distance between the image centers 0.0389 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:42:50.965 -10:00:26.84
Second-epoch image center 13:42:56.340 -09:58:28.47
Angular distance between the image centers 0.0396 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:42:54.071 -09:58:14.56
Second-epoch second image center 13:42:56.340 -09:58:28.47
Angular distance between the image centers 0.01008 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits &> /tmp/tmp.pxfVdrMZg8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits &> /tmp/tmp.71vOtbLPwI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits &> /tmp/tmp.XCMtvdqJha
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits &> /tmp/tmp.PoZPzXTl5O
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
Found non-empty wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits and wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
The reference image (wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits) and catalog (wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat) found
'wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat' -> 'wcsmag.cat'
Read 31003 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6003 to 213.7472 deg, Dec -15.2838 to -4.6412 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 197.6003 to 213.7472 deg, Dec -15.2838 to -4.6412 deg
Loaded 4397 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3514 out of 3762 total matches.
Matched with Tycho-2 3762 out of 31003 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.780085
a=0.000000 b=1.000000 c=22.780085
From vast_summary.log: estimated ref. image limiting mag.: -7.80
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.98
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.98
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 48 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
2.3 pix Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
2.8 pix fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
2.6 pix fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
Limiting magnitude estimates:
15.0 mag. Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
15.0 mag. Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
14.9 mag. fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
15.0 mag. fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.pxfVdrMZg8 (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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits' -> 'wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1266, passed=30997
Got 30997 stars (including 29699 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat
util/solve_plate_with_UCAC5 got 30997 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 30630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 30629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 30629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits -region wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.71vOtbLPwI (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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits' -> 'wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1340, passed=30818
Got 30818 stars (including 29441 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat
util/solve_plate_with_UCAC5 got 30818 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 30443 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 30443 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 30443 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits -region wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.XCMtvdqJha (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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1991, passed=28679
Got 28679 stars (including 26661 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat
util/solve_plate_with_UCAC5 got 28679 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 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 28245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 28246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 28246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits -region wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.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.PoZPzXTl5O (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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2083, passed=29692
Got 29692 stars (including 27586 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat
util/solve_plate_with_UCAC5 got 29692 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 29169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.3 to -4.6)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 29169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 29169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits -region wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/wcs_Vir-12-Q2b1x1_2026-02-27_03-46-31_20.00sec_-14.90C_LIGHT_0204.fits
Saving fully-calibrated image wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/wcs_Vir-12-Q2b1x1_2026-02-27_03-47-17_20.00sec_-14.90C_LIGHT_0205.fits
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-47-22_20.00sec_-4.90C_LIGHT_0243.fits
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.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_2026-04-09_CI_Vir-12-Q2b1x1_021532_TTUQ2b1x1_19325_JGc1rtC2/wcs_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244.fits
Preparing the HTML report for the field Vir-12-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52092.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out51907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52215.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51840_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 51840_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:52:15.71 -05:46:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 4.590 3620759655045211008 208.06615619262 -05.78206947411 14.7287 14.4060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51844_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 51844_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:28:00.75 -09:32:55.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51898_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 51898_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:16:57.55 -10:12:46.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51907_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
Preparing report for the candidate 51907_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51928_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
Preparing report for the candidate 51928_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51948_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 51948_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:25:24.13 -11:11:15.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51955_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 51955_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:23:08.44 -05:46:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.104 3634614360548939520 200.78458021740 -05.77863285749 13.1904 12.6573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51968_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 51968_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 52062_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52062_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:30:33.69 -06:05:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52092_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52092_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:27:09.52 -11:47:17.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)
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Considering the candidate 52095_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52095_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:30:16.78 -10:03:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52108_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52108_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:21:16.79 -07:05:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.640 3631415709425012096 200.31989853599 -07.09844367183 14.3262 13.5885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52112_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
Preparing report for the candidate 52112_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
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Considering the candidate 52132_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52132_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52141_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52141_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:17:04.41 -08:58:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 2.182 3624926701035507968 199.26878556857 -08.96875607539 15.0235 14.6848 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52144_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52144_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:24:30.56 -07:00:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 3.920 3631453191604281088 201.12819283985 -07.00831540186 14.7389 14.2358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52155_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52155_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:16:12.93 -06:57:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.840 3628466028965314688 199.05358144034 -06.96599669977 14.3819 13.6105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52158_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52158_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:20:42.25 -12:17:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 0.242 3611065535901271936 200.17608305114 -12.29860936013 14.3910 13.5996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52164_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52164_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:17:00.26 -09:28:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.858 3624478924925095040 199.25070369341 -09.46727176922 14.5585 14.0372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52166_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52166_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:26:41.65 -13:55:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 0.608 3608413445135733376 201.67346450201 -13.92076526503 14.3815 13.8334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52167_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52167_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:17:52.36 -12:41:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 0.600 3609575143594529152 199.46830760538 -12.68401673884 14.3549 13.7248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52170_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52170_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:18:06.49 -09:51:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 2.524 3623698065510952320 199.52691921038 -09.86469810098 14.3718 13.5575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52175_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52175_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:16:47.51 -12:45:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.388 3609570749843381632 199.19757146242 -12.75680085135 14.0317 13.3130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52177_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52177_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:17:03.10 -11:00:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.348 3623467168069177600 199.26293049943 -11.00067898080 14.4426 13.8744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52190_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52190_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:18:18.57 -07:35:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.867 3625368945228038016 199.57782138245 -07.59032628361 14.7138 14.3871 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52195_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52195_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:22:13.18 -06:51:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 1.460 3631429689542706048 200.55507475105 -06.86284623527 14.6188 14.1143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52197_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52197_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:26:23.31 -11:38:34.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)
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Considering the candidate 52198_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52198_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:16:37.07 -12:44:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.265 3609582741392072448 199.15472365617 -12.74548788297 14.6422 14.1475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52200_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52200_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:23:28.52 -05:46:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 1.147 3634986545234876288 200.86898665834 -05.78158532924 14.6841 14.1904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52201_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52201_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:48:11.30 -11:28:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.359 3613478139290772224 207.04733421614 -11.47500853677 14.3463 13.6634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52207_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52207_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:18:53.71 -12:46:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 2.165 3609524364196645888 199.72328494089 -12.78312042417 14.5593 14.0861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52208_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52208_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:17:29.02 -12:10:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.419 3621636584288178176 199.37090845834 -12.17528303002 14.4965 13.9442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52215_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
Preparing report for the candidate 52215_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
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Considering the candidate 52232_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52232_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:35:55.60 -14:03:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52233_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52233_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:18:50.02 -08:04:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 0.646 3625271638448939904 199.70859329901 -08.07034593751 14.4093 13.8653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52237_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52237_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:20:29.62 -12:08:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.847 3611116796335492480 200.12296276654 -12.14961860946 14.6175 14.1097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52249_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52249_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:40:16.69 -07:11:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 2.306 3630654194543585664 205.07017072640 -07.19843865666 14.1906 13.1841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52250_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52250_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:34:30.07 -07:28:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52255_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52255_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:22:53.73 -12:39:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 0.690 3610840101657835136 200.72400973746 -12.65747291892 14.5633 13.9437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52262_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52262_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:22:48.52 -10:54:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 0.069 3623329522957227264 200.70217739220 -10.90857154686 14.4645 13.8807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52267_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52267_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:42:36.81 -07:08:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.484 3620146746032450176 205.65375283461 -07.14110658746 14.4230 13.8136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52298_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52298_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:32:13.15 -12:50:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 1.919 3609906616286050048 203.05533719549 -12.84161656047 14.7961 14.3121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52301_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52301_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:29:22.06 -12:25:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52302_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52302_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:25:33.81 -13:08:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52306_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 52306_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 21056_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 21056_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:35:16.12 -06:58:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07966_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 07966_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks
**** FOUND 13:32:31.47 -12:17:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26170_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244
The candidate 26170_fd_Vir-12-Q2b1x1_2026-04-09_01-48-09_20.00sec_-4.90C_LIGHT_0244 did not pass the final checks