This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 20.2308 2461180.7308 13.32 12:20:42.52 +02:22:50.5
285.07263 64.18172 galactic Vir Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.238 Hypatia 0 0 0 13.3 -0 0
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:20:42.52 +02:22:50.5: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:20:42.52 +02:22:50.5: 15.76 +/- 99.00 upperlimit
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 05 20.2309* 12 20 42.52 +02 22 50.5 13.3 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461180.7308,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260520.2308 13.32CV 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 05 20.2308 2461180.7308 13.89 13:19:04.68 +08:06:56.1
323.20219 69.89208 galactic Vir Second-epoch detections are separated by 1.2" and 6.4 pix
The object was found in VSX 1" CSS_J131904.7+080654
Type: RRAB
# Max. Min./Amp. JD0 Period
14.844 CV Y 1.250 CV 2455242.01110 0.462260000000
The object was not found in astcheck.
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 13:19:04.68 +08:06:56.1: 15.22 +/- 0.21 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 13:19:04.68 +08:06:56.1: 15.90 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.22 +/- 0.21
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 05 20.2309* 13 19 04.68 +08 06 56.1 13.9 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
CSS_J131904.7+080654,2461180.7308,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CSS_J131904.7+080654 20260520.2308 13.89CV 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: 2461146.76361255 16.04.2026 06:19:26.124 /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
First image: 2461146.76361255 16.04.2026 06:19:26.124 /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
Last image: 2461180.73107742 20.05.2026 05:32:35.089 /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5740
Objects passed selection criteria: 5738
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 5614.25
Average stars matched: 5461 (97.2703 %)
Memory usage VmPeak: 111724 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 19 15:05:05 CDT 2026
VaST build number 1.0rc89-63-g0e0f9022
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-19)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed May 20 00:35:38 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: 2461146.76361255 16.04.2026 06:19:26.124 /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
First image: 2461146.76361255 16.04.2026 06:19:26.124 /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
Last image: 2461180.73107742 20.05.2026 05:32:35.089 /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 21
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 27712
Objects passed selection criteria: 27666
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 26251
Average stars matched: 24806 (94.4954 %)
Memory usage VmPeak: 131688 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 19 15:05:05 CDT 2026
VaST build number 1.0rc89-63-g0e0f9022
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-19)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed May 20 00:36:52 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
SExtractor catalog cache: saved Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.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: 2461180.73061947
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
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits'
wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits exists and is non-empty
Saving wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits to local_wcs_cache/
'wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits' -> 'local_wcs_cache/wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits'
wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits exists and is non-empty
Saving wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits to local_wcs_cache/
'wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits' -> 'local_wcs_cache/wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits'
wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits exists and is non-empty
Saving wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits to local_wcs_cache/
'wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits' -> 'local_wcs_cache/wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:51:26.634 +06:00:59.74 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits (1st new image)
verification OK: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:51:38.924 +06:03:04.69 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:51:26.634 +06:00:59.74
Second-epoch image center 12:51:38.924 +06:03:04.69
Angular distance between the image centers 0.0616 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits (2nd new image)
verification OK: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:51:40.987 +06:02:43.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:51:26.634 +06:00:59.74
Second-epoch image center 12:51:40.987 +06:02:43.51
Angular distance between the image centers 0.0661 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 12:51:38.924 +06:03:04.69
Second-epoch second image center 12:51:40.987 +06:02:43.51
Angular distance between the image centers 0.01038 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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits &> /tmp/tmp.8JF67edJ92
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits &> /tmp/tmp.GRItDphNeF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits &> /tmp/tmp.VilarfeQ97
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits &> /tmp/tmp.Y60SiXCKkw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits and wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits and wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat
Found non-empty wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits and wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat
The reference image (wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits) and catalog (wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat) found
'wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat' -> 'wcsmag.cat'
Read 5828 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 184.8413 to 200.7535 deg, Dec +0.6684 to +11.3112 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 184.8413 to 200.7535 deg, Dec 0.6684 to 11.3112 deg
Loaded 3689 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): 3029 out of 3129 total matches.
Matched with Tycho-2 3129 out of 5828 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.848600
a=0.000000 b=1.000000 c=22.848600
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.27
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.27
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5828 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 184.8413 to 200.7535 deg, Dec +0.6684 to +11.3112 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 184.8413 to 200.7535 deg, Dec 0.6684 to 11.3112 deg
Loaded 3689 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): 3029 out of 3129 total matches.
Matched with Tycho-2 3129 out of 5828 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits:
Forced-photometry filter: calibrated wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits -> calib.txt_param_ref_wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits (aperture=6.5)
Read 5560 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.0347 to 201.1957 deg, Dec +0.1686 to +11.7896 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 185.0347 to 201.1957 deg, Dec 0.1686 to 11.7896 deg
Loaded 4084 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): 582 out of 614 total matches.
Matched with Tycho-2 614 out of 5560 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits:
Forced-photometry filter: calibrated wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits -> calib.txt_param_ref_wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
2.2 pix Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
4.3 pix fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
4.4 pix fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
2.3 pix wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
2.2 pix wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
Limiting magnitude estimates:
15.3 mag. Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
15.3 mag. Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
14.8 mag. fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
14.8 mag. fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
All-image limiting magnitude estimate: 14.8 (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.8JF67edJ92 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits 565.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits' -> 'wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
Checking if the catalog wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat corresponding to the image wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat corresponding to the image wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
WCS catalog name: wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=353, passed=5828
Got 5828 stars (including 5473 good ones) from the SExtractor catalog wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 5828 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 5768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 5768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 5768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits N_match=980 sigma_overall_arcsec=0.385 sigma_q1_arcsec=0.304 sigma_q2_arcsec=0.426 sigma_q3_arcsec=0.330 sigma_q4_arcsec=0.480 n_q1=249 n_q2=243 n_q3=229 n_q4=259 worst_quadrant_to_overall_ratio=1.247
The image catalog is written to wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits -region wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.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.GRItDphNeF (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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.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-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits' -> 'wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
WCS_IMAGE_NAME=wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
WCS-calibrated image found: wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
Checking if the catalog wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat corresponding to the image wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits alredy exist and is non-empty...
Catalog wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat corresponding to the image wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
WCS catalog name: wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=408, passed=5560
Got 5560 stars (including 5144 good ones) from the SExtractor catalog wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat
util/solve_plate_with_UCAC5 got 5560 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 916.3'
Seting catalog search parameters based on the expected field of view 916.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012726 (45.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010181 (36.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.8)
Done reading UCAC5 zone files...
Matched 523 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 519 matched stars entering correct_measured_positions(), 502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.14"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 519 matched stars entering correct_measured_positions(), 2983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.8)
Done reading UCAC5 zone files...
Matched 564 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 562 matched stars entering correct_measured_positions(), 3008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.09"
Accuracy estimation diagnostic: 562 matched stars entering correct_measured_positions(), 3203 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.21"
Excluding outliers - 562 stars left (next iteration limit 570)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits N_match=562 sigma_overall_arcsec=4.041 sigma_q1_arcsec=3.681 sigma_q2_arcsec=13.941 sigma_q3_arcsec=3.812 sigma_q4_arcsec=11.688 n_q1=249 n_q2=27 n_q3=240 n_q4=46 worst_quadrant_to_overall_ratio=3.450
The image catalog is written to wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits -region wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.VilarfeQ97 (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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
WCS_IMAGE_NAME=wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
WCS-calibrated image found: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
Checking if the catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat corresponding to the image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat corresponding to the image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
WCS catalog name: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=242, passed=5641
Got 5641 stars (including 5397 good ones) from the SExtractor catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat
util/solve_plate_with_UCAC5 got 5641 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits N_match=976 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.353 sigma_q2_arcsec=0.352 sigma_q3_arcsec=0.263 sigma_q4_arcsec=0.322 n_q1=263 n_q2=220 n_q3=231 n_q4=262 worst_quadrant_to_overall_ratio=1.092
The image catalog is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits -region wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.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.Y60SiXCKkw (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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
WCS_IMAGE_NAME=wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
WCS-calibrated image found: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
Checking if the catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat corresponding to the image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat corresponding to the image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
WCS catalog name: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=231, passed=5620
Got 5620 stars (including 5384 good ones) from the SExtractor catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat
util/solve_plate_with_UCAC5 got 5620 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits N_match=976 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.353 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.326 n_q1=264 n_q2=220 n_q3=230 n_q4=262 worst_quadrant_to_overall_ratio=1.098
The image catalog is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits -region wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits sigma_overall=0.385 worst_q_ratio=1.247
ref2=Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits sigma_overall=4.041 worst_q_ratio=3.450
new1=fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits sigma_overall=0.324 worst_q_ratio=1.092
new2=fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits sigma_overall=0.329 worst_q_ratio=1.098
reference average sigma_overall=2.213 worst_q_ratio=2.3485
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226_astrometric_residuals.png (980 matched stars from wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219_astrometric_residuals.png (562 matched stars from wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152_astrometric_residuals.png (976 matched stars from wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153_astrometric_residuals.png (976 matched stars from wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits'
Saving fully-calibrated image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits'
Preparing the HTML report for the field Vir-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:59:37.46 +07:44:38.5: 12.38 +/- 0.01 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:34:08.60 +02:39:13.0: 12.06 +/- 0.01 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:59:37.46 +07:44:38.5: 12.40 +/- 0.01 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:34:08.60 +02:39:13.0: 15.81 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter REJECTED candidate at 12:34:08.60 +02:39:13.0: ref_mag=12.06 +/- 0.01 new_mean_mag=11.8014 delta=0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 12:59:37.46 +07:44:38.5: ref_mag=12.39 +/- 0.01 new_mean_mag=12.3387 delta=0.05 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
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Considering the candidate 20443_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 20443_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
**** FOUND 13:17:36.27 +05:26:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20448_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 20448_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
**** FOUND 13:16:16.62 +06:29:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20452_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 20452_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 20453_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 20453_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 03106_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 03106_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
**** FOUND 12:51:05.73 +05:33:11.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Vir-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
SExtractor catalog cache: saved Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits exists and is non-empty
wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits exists and is non-empty
wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits exists and is non-empty
wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:51:26.634 +06:00:59.74 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits (1st new image)
verification OK: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:51:38.924 +06:03:04.69 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:51:26.634 +06:00:59.74
Second-epoch image center 12:51:38.924 +06:03:04.69
Angular distance between the image centers 0.0616 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits (2nd new image)
verification OK: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 12:51:40.987 +06:02:43.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:51:26.634 +06:00:59.74
Second-epoch image center 12:51:40.987 +06:02:43.51
Angular distance between the image centers 0.0661 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 12:51:38.924 +06:03:04.69
Second-epoch second image center 12:51:40.987 +06:02:43.51
Angular distance between the image centers 0.01038 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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits &> /tmp/tmp.jr4qoeF6AE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits &> /tmp/tmp.qFRNAkCuXf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits &> /tmp/tmp.ESJ3hnl5pP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits &> /tmp/tmp.Ngk6ecx6hr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits and wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits and wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat
Found non-empty wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits and wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat
The reference image (wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits) and catalog (wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat) found
'wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat' -> 'wcsmag.cat'
Read 29468 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 184.8321 to 200.7627 deg, Dec +0.6380 to +11.3144 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 184.8321 to 200.7627 deg, Dec 0.6380 to 11.3144 deg
Loaded 3701 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): 2940 out of 3152 total matches.
Matched with Tycho-2 3152 out of 29468 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.739300
a=0.000000 b=1.000000 c=22.739300
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29468 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 184.8321 to 200.7627 deg, Dec +0.6380 to +11.3144 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 184.8321 to 200.7627 deg, Dec 0.6380 to 11.3144 deg
Loaded 3701 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): 2940 out of 3152 total matches.
Matched with Tycho-2 3152 out of 29468 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits:
Forced-photometry filter: calibrated wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits -> calib.txt_param_ref_wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits (aperture=5.1)
Read 31436 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 185.0028 to 201.2172 deg, Dec +0.1686 to +11.8173 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 185.0028 to 201.2172 deg, Dec 0.1686 to 11.8173 deg
Loaded 4110 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): 572 out of 626 total matches.
Matched with Tycho-2 626 out of 31436 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits:
Forced-photometry filter: calibrated wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits -> calib.txt_param_ref_wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 18 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
2.1 pix Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
3.8 pix fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
3.8 pix fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
2.2 pix wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
2.1 pix wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
Limiting magnitude estimates:
15.4 mag. Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
15.5 mag. Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
14.9 mag. fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
14.9 mag. fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.3 (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.jr4qoeF6AE (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits 565.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.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-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits' -> 'wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
Checking if the catalog wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat corresponding to the image wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat corresponding to the image wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits
WCS catalog name: wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1250, passed=29455
Got 29455 stars (including 28173 good ones) from the SExtractor catalog wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 29455 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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 29148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 29147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 29147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits N_match=979 sigma_overall_arcsec=0.402 sigma_q1_arcsec=0.294 sigma_q2_arcsec=0.498 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.463 n_q1=255 n_q2=239 n_q3=232 n_q4=253 worst_quadrant_to_overall_ratio=1.239
The image catalog is written to wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits -region wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.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.qFRNAkCuXf (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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.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-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits' -> 'wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
WCS_IMAGE_NAME=wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
WCS-calibrated image found: wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
Checking if the catalog wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat corresponding to the image wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits alredy exist and is non-empty...
Catalog wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat corresponding to the image wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits
WCS catalog name: wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1166, passed=31421
Got 31421 stars (including 30205 good ones) from the SExtractor catalog wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat
util/solve_plate_with_UCAC5 got 31421 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 916.3'
Seting catalog search parameters based on the expected field of view 916.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012726 (45.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010181 (36.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 511 (Dec 0.2 to 11.8)
Done reading UCAC5 zone files...
Matched 522 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 519 matched stars entering correct_measured_positions(), 502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.09"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 519 matched stars entering correct_measured_positions(), 16899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 511 (Dec 0.2 to 11.8)
Done reading UCAC5 zone files...
Matched 565 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 562 matched stars entering correct_measured_positions(), 16925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.39"
Accuracy estimation diagnostic: 562 matched stars entering correct_measured_positions(), 18276 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.22"
Excluding outliers - 562 stars left (next iteration limit 570)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits N_match=562 sigma_overall_arcsec=3.900 sigma_q1_arcsec=3.602 sigma_q2_arcsec=17.891 sigma_q3_arcsec=3.603 sigma_q4_arcsec=11.276 n_q1=246 n_q2=28 n_q3=241 n_q4=47 worst_quadrant_to_overall_ratio=4.587
The image catalog is written to wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits -region wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ESJ3hnl5pP (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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
WCS_IMAGE_NAME=wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
WCS-calibrated image found: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
Checking if the catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat corresponding to the image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat corresponding to the image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
WCS catalog name: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=841, passed=22524
Got 22524 stars (including 21667 good ones) from the SExtractor catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat
util/solve_plate_with_UCAC5 got 22524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 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 451 to 510 (Dec 0.3 to 11.7)
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(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 22315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
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(), 22317 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 22317 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits N_match=977 sigma_overall_arcsec=0.326 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.349 sigma_q3_arcsec=0.280 sigma_q4_arcsec=0.334 n_q1=261 n_q2=218 n_q3=235 n_q4=263 worst_quadrant_to_overall_ratio=1.095
The image catalog is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits -region wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.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.Ngk6ecx6hr (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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
WCS_IMAGE_NAME=wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
WCS-calibrated image found: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
Checking if the catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat corresponding to the image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat corresponding to the image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
WCS catalog name: wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=832, passed=22501
Got 22501 stars (including 21647 good ones) from the SExtractor catalog wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat
util/solve_plate_with_UCAC5 got 22501 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 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 451 to 510 (Dec 0.3 to 11.7)
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(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 22314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
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(), 22313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 22313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits N_match=977 sigma_overall_arcsec=0.335 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.353 sigma_q3_arcsec=0.291 sigma_q4_arcsec=0.340 n_q1=264 n_q2=217 n_q3=233 n_q4=263 worst_quadrant_to_overall_ratio=1.076
The image catalog is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits -region wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-31-55_20.00sec_-0.00C_LIGHTs_0152.fits
Saving fully-calibrated image wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.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_2026-05-20_CI_Vir-03-Q1b1x1_003324_TTUQ1b1x1_3334981_kZpZmBzx/wcs_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153.fits
Preparing the HTML report for the field Vir-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:26:56.89 +06:56:41.6: 14.42 +/- 0.08 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:21:48.14 +03:15:49.7: 14.33 +/- 0.09 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:26:35.93 +03:57:55.8: 13.63 +/- 0.04 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 13:12:04.42 +02:06:23.3: 13.91 +/- 0.07 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 13:02:26.87 +05:10:43.9: 12.22 +/- 0.01 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:24:53.92 +03:59:20.5: 14.66 +/- 0.11 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:29:28.13 +08:45:00.6: 12.73 +/- 0.02 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 13:19:04.68 +08:06:56.1: 15.22 +/- 0.21 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:20:42.52 +02:22:50.5: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:26:56.89 +06:56:41.6: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:26:35.93 +03:57:55.8: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:24:53.92 +03:59:20.5: 15.92 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.42 +/- 0.08
Forced photometry reference-image weighted average: 13.63 +/- 0.04
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:21:48.14 +03:15:49.7: 15.84 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 12:26:56.89 +06:56:41.6: ref_mag=14.42 +/- 0.08 new_mean_mag=14.5815 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 12:26:35.93 +03:57:55.8: ref_mag=13.63 +/- 0.04 new_mean_mag=13.1165 delta=0.51 (need > 0.90)
Forced photometry reference-image weighted average: 14.66 +/- 0.11
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 13:02:26.87 +05:10:43.9: 12.31 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 12:24:53.92 +03:59:20.5: ref_mag=14.66 +/- 0.11 new_mean_mag=14.5040 delta=0.16 (need > 0.90)
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 13:12:04.42 +02:06:23.3: 15.38 +/- 0.24 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:29:28.13 +08:45:00.6: 16.02 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.33 +/- 0.09
Forced photometry filter REJECTED candidate at 12:21:48.14 +03:15:49.7: ref_mag=14.33 +/- 0.09 new_mean_mag=14.0722 delta=0.26 (need > 0.90)
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Forced photometry reference-image weighted average: 14.02 +/- 0.06
Forced photometry filter REJECTED candidate at 13:02:26.87 +05:10:43.9: ref_mag=12.26 +/- 0.01 new_mean_mag=12.2342 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 12:29:28.13 +08:45:00.6: ref_mag=12.73 +/- 0.02 new_mean_mag=12.3087 delta=0.42 (need > 0.90)
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:26:09.17 +03:43:09.2: 15.45 +/- 0.23 detection
Forced photometry filter REJECTED candidate at 13:12:04.42 +02:06:23.3: ref_mag=14.02 +/- 0.06 new_mean_mag=14.0663 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 13:19:04.68 +08:06:56.1: 15.90 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.22 +/- 0.21
Forced photometry filter KEPT candidate at 13:19:04.68 +08:06:56.1: ref_mag=15.22 +/- 0.21 new_mean_mag=13.8827 delta=1.33 (need > 0.90)
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:20:42.52 +02:22:50.5: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:26:09.17 +03:43:09.2: 15.98 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.45 +/- 0.23
Forced photometry filter REJECTED candidate at 12:26:09.17 +03:43:09.2: ref_mag=15.45 +/- 0.23 new_mean_mag=14.6913 delta=0.75 (need > 0.90)
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 13:03:51.80 +09:25:33.8: 15.77 +/- 0.29 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_01-19-26_20.00sec_-4.90C_LIGHT_0226.fits at 12:38:40.52 +10:26:04.6: 14.78 +/- 0.11 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 13:03:51.80 +09:25:33.8: 15.57 +/- 0.25 detection
Forced photometry on wcs_Vir-03-Q1b1x1_2026-04-16_02-07-49_20.00sec_-5.00C_LIGHTs_0219.fits at 12:38:40.52 +10:26:04.6: 16.08 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.66 +/- 0.19
Forced photometry filter REJECTED candidate at 13:03:51.80 +09:25:33.8: ref_mag=15.66 +/- 0.19 new_mean_mag=14.9128 delta=0.74 (need > 0.90)
Forced photometry reference-image weighted average: 14.78 +/- 0.11
Forced photometry filter REJECTED candidate at 12:38:40.52 +10:26:04.6: ref_mag=14.78 +/- 0.11 new_mean_mag=14.5701 delta=0.21 (need > 0.90)
Adding exclusion_list_local.txt__out34956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35028.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 34869_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 34869_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 34872_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 34872_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 34883_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 34883_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 34884_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 34884_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 34886_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 34886_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
**** FOUND 13:17:10.37 +01:31:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34889_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 34889_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 34893_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 34893_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
**** FOUND 13:17:36.27 +05:26:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34904_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 34904_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 34908_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 34908_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 34925_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 34925_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
**** FOUND 12:37:04.24 +08:46:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34956_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
Preparing report for the candidate 34956_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
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Considering the candidate 35012_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 35012_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 35028_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
Preparing report for the candidate 35028_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
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Considering the candidate 35210_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 35210_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 35253_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 35253_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 35259_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 35259_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
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Considering the candidate 20425_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 20425_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks
**** FOUND 12:45:20.24 +03:58:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15460_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153
The candidate 15460_fd_Vir-03-Q1b1x1_2026-05-20_00-32-35_20.00sec_-0.00C_LIGHTs_0153 did not pass the final checks