This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z
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 09.3267* 13 32 50.40 +11 15 18.4 13.1 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,2461139.8267,13.05,0.05,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 20260409.3267 13.05CV 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 09.3267* 13 26 55.53 +12 29 40.1 14.0 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8267,14.00,0.05,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 20260409.3267 14.00CV 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
Mean magnitude and position on the discovery images:
2026 04 09.3267 2461139.8267 14.89 13:33:05.04 +14:12:17.1
341.92825 73.83503 galactic Vir Second-epoch detections are separated by 3.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3741661987995737344 | 13:33:05.04 +14:12:17.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.972+/-0.107 (M)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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 09.3267* 13 33 05.04 +14 12 17.1 14.9 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
Large-amplitude variable Gaia DR2 3741661987995737344,2461139.8267,14.89,0.05,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
Large-amplitude variable Gaia DR2 3741661987995737344 20260409.3267 14.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
First image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Last image: 2461139.82698801 09.04.2026 07:50:41.764 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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): 4638
Objects passed selection criteria: 4633
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: 4364.5
Average stars matched: 4242.5 (97.2047 %)
Memory usage VmPeak: 110952 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 03:07:49 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
First image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Last image: 2461139.82698801 09.04.2026 07:50:41.764 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 66
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.26
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: 16 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): 25377
Objects passed selection criteria: 25306
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 23860.2
Average stars matched: 22826.8 (95.6685 %)
Memory usage VmPeak: 128804 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 03:08:51 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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat to cache
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.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: 2461139.82641889
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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits exists and is non-empty
Saving wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits to local_wcs_cache/
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> 'local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits exists and is non-empty
Saving wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits to local_wcs_cache/
'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> 'local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits exists and is non-empty
Saving wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits to local_wcs_cache/
'wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits' -> 'local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits'
wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits exists and is non-empty
Saving wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits to local_wcs_cache/
'wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits' -> 'local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:52.170 +14:01:01.65
Angular distance between the image centers 0.0439 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 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:54.968 +14:00:35.65
Angular distance between the image centers 0.0307 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:19:52.170 +14:01:01.65
Second-epoch second image center 13:19:54.968 +14:00:35.65
Angular distance between the image centers 0.01342 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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits &> /tmp/tmp.MiDWQkvIGW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits &> /tmp/tmp.BzXR7nHGqr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits &> /tmp/tmp.7rr6y4mify
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits &> /tmp/tmp.mQzs8yYIj0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
The reference image (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits) and catalog (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat) found
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat' -> 'wcsmag.cat'
Read 5868 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 191.7478 to 208.6496 deg, Dec +8.1787 to +19.6104 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 191.7478 to 208.6496 deg, Dec 8.1787 to 19.6104 deg
Loaded 4013 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): 2880 out of 3002 total matches.
Matched with Tycho-2 3002 out of 5868 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.944237
a=0.000000 b=1.000000 c=22.944237
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
2.3 pix Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
2.4 pix fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
2.4 pix fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
Limiting magnitude estimates:
15.4 mag. Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
15.4 mag. Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
15.3 mag. fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
15.3 mag. fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.3 (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.MiDWQkvIGW (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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/util/wcs_image_calibration.sh: line 129: echo: write error: Broken pipe
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=363, passed=5868
Got 5868 stars (including 5502 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
util/solve_plate_with_UCAC5 got 5868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 490 to 550 (Dec 8.2 to 19.6)
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(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.2 to 19.6)
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(), 5772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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.BzXR7nHGqr (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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=372, passed=5872
Got 5872 stars (including 5497 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 5872 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 490 to 550 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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.7rr6y4mify (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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=299, passed=5606
Got 5606 stars (including 5301 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat
util/solve_plate_with_UCAC5 got 5606 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 493 to 548 (Dec 8.6 to 19.3)
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(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
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(), 5528 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5528 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits -region wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.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.mQzs8yYIj0 (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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=302, passed=5542
Got 5542 stars (including 5237 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat
util/solve_plate_with_UCAC5 got 5542 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 492 to 548 (Dec 8.6 to 19.3)
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(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5462 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
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(), 5463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits -region wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
Saving fully-calibrated image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits'
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits'
Preparing the HTML report for the field Vir-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Vir-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat to cache
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Creating symlink local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits exists and is non-empty
wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits exists and is non-empty
wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits exists and is non-empty
wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:52.170 +14:01:01.65
Angular distance between the image centers 0.0439 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 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:54.968 +14:00:35.65
Angular distance between the image centers 0.0307 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:19:52.170 +14:01:01.65
Second-epoch second image center 13:19:54.968 +14:00:35.65
Angular distance between the image centers 0.01342 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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits &> /tmp/tmp.oXU4YX35zp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits &> /tmp/tmp.ReWutBdtMo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits &> /tmp/tmp.ry3S6EFvNx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits &> /tmp/tmp.06QB5AxKtP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
The reference image (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits) and catalog (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat) found
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat' -> 'wcsmag.cat'
Read 30168 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 191.7108 to 208.6501 deg, Dec +8.0896 to +19.6104 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 191.7108 to 208.6501 deg, Dec 8.0896 to 19.6104 deg
Loaded 4057 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): 2777 out of 3023 total matches.
Matched with Tycho-2 3023 out of 30168 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.816035
a=0.000000 b=1.000000 c=22.816035
From vast_summary.log: estimated ref. image limiting mag.: -7.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 25 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
2.2 pix Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
2.3 pix fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
2.2 pix fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
Limiting magnitude estimates:
15.6 mag. Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
15.6 mag. Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
15.4 mag. fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
15.5 mag. fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.8 (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.oXU4YX35zp (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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1276, passed=30154
Got 30154 stars (including 28848 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
util/solve_plate_with_UCAC5 got 30154 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 490 to 550 (Dec 8.1 to 19.6)
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(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 29813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
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(), 29814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 29814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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.ReWutBdtMo (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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1283, passed=30242
Got 30242 stars (including 28923 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 30242 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 490 to 550 (Dec 8.1 to 19.6)
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(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 29812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
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(), 29812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 29812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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.ry3S6EFvNx (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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1122, passed=27701
Got 27701 stars (including 26542 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat
util/solve_plate_with_UCAC5 got 27701 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 492 to 548 (Dec 8.6 to 19.3)
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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 27292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
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(), 27288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 27288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits -region wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.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.06QB5AxKtP (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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1230, passed=28240
Got 28240 stars (including 26978 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat
util/solve_plate_with_UCAC5 got 28240 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 492 to 548 (Dec 8.6 to 19.3)
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(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 27783 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
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(), 27785 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 27785 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits -region wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Saving fully-calibrated image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-49-52_20.00sec_-5.00C_LIGHT_0287.fits
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.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-01-Q2b1x1_025338_TTUQ2b1x1_23330_XoaMlY1Z/wcs_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288.fits
Preparing the HTML report for the field Vir-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52630.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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 51841_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 51841_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:02:52.44 +10:11:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 0.901 3734525504696418560 195.71833051046 +10.19598021002 14.2882 13.7591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51843_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 51843_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:31:28.81 +13:40:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.125 3740135797136944512 202.87020591792 +13.66871323656 14.4335 13.9760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52091_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
Preparing report for the candidate 52091_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52172_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52172_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:43:51.88 +13:35:59.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52300_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52300_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:10:01.55 +16:10:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52329_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52329_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:21:49.21 +10:44:21.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52364_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
Preparing report for the candidate 52364_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52430_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52430_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:07:11.63 +10:16:02.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52468_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52468_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:30:16.50 +12:12:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.51, MAG_FAINT_SEARCH_LIMIT=15.49)GAIADR2_OUTPUT=# 0.888 3739680668042399872 202.56889983205 +12.20730146651 14.4430 13.7938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52516_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52516_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:18:46.25 +09:50:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 2.151 3732929426129713664 199.69215800773 +09.84066776404 14.5034 13.8803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52538_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52538_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:05:32.96 +12:49:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.707 3737715187927847296 196.38802482873 +12.82786137540 15.2527 14.6147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52571_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52571_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:12:44.92 +18:11:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 4.913 3938022360852572288 198.18836118450 +18.19928577809 14.8682 14.7199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52577_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52577_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:44:43.35 +10:09:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 0.643 3725551977984782080 206.18080086152 +10.16046019343 14.4569 13.8263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52608_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52608_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:17:12.44 +09:49:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52630_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
Preparing report for the candidate 52630_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52644_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52644_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:17:09.22 +09:50:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 2.782 3732568683236604288 199.28785491719 +09.84112722707 14.9861 14.4759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52678_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52678_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:40:34.36 +10:04:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 3.086 3726245013907659136 205.14396224014 +10.07984623383 15.1969 14.5429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52702_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52702_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:40:06.01 +14:02:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52718_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52718_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:47:47.22 +12:47:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.379 3728344290842813568 206.94702663430 +12.79800572618 13.8260 12.6220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52744_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52744_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:11:14.56 +09:42:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 0.690 3732705984751520256 197.81069815257 +09.71168919262 14.9078 14.2698 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52783_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52783_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:29:43.69 +15:02:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.060 3744824595754006144 202.43197493829 +15.03934300118 15.0130 14.5219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52793_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52793_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:32:41.56 +10:36:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.607 3738156813645359104 203.17287257413 +10.61002095872 14.9265 14.3792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52842_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52842_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:14:39.49 +17:11:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.237 3936953979146081792 198.66489645626 +17.19689040455 15.6213 15.2374 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52849_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52849_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks
**** FOUND 13:22:19.23 +18:10:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.900 3938593247903806592 200.57964862112 +18.17046599049 15.1615 14.4501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52890_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288
The candidate 52890_fd_Vir-01-Q2b1x1_2026-04-09_02-50-41_20.00sec_-4.90C_LIGHT_0288 did not pass the final checks