This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.3721* 13 31 55.05 +11 24 29.2 13.0 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.8721,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.3721 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.3721* 13 25 56.74 +12 32 33.9 14.0 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.8721,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.3721 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.3721* 13 18 36.78 +15 18 39.9 10.9 U Com 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
QT Com,2461140.8721,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
QT Com 20260410.3721 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
First image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Last image: 2461140.87241929 10.04.2026 08:56:07.027 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 4639
Objects passed selection criteria: 4632
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 4367.25
Average stars matched: 4239 (97.0634 %)
Memory usage VmPeak: 110924 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 04:52:45 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
First image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Last image: 2461140.87241929 10.04.2026 08:56:07.027 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 52
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.26
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 13 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 24482
Objects passed selection criteria: 24415
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: 22507
Average stars matched: 21664.5 (96.2567 %)
Memory usage VmPeak: 128556 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 04:53:50 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat to cache
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461140.87180931
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits exists and is non-empty
Saving wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits to local_wcs_cache/
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> 'local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits exists and is non-empty
Saving wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits to local_wcs_cache/
'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> 'local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits exists and is non-empty
Saving wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits to local_wcs_cache/
'wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits' -> 'local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits'
wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits exists and is non-empty
Saving wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits to local_wcs_cache/
'wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits' -> 'local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:52.079 +14:01:57.69
Angular distance between the image centers 0.0557 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:53.815 +14:02:38.36
Angular distance between the image centers 0.0618 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:19:52.079 +14:01:57.69
Second-epoch second image center 13:19:53.815 +14:02:38.36
Angular distance between the image centers 0.01330 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits &> /tmp/tmp.vrtnKxgI9f
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits &> /tmp/tmp.dEe446T9AQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits &> /tmp/tmp.ueRWyRtfN3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits &> /tmp/tmp.G8dw6dDL3z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
The reference image (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits) and catalog (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat) found
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat' -> 'wcsmag.cat'
Read 5868 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 191.7478 to 208.6496 deg, Dec +8.1787 to +19.6104 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 191.7478 to 208.6496 deg, Dec 8.1787 to 19.6104 deg
Loaded 4013 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2880 out of 3002 total matches.
Matched with Tycho-2 3002 out of 5868 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.944237
a=0.000000 b=1.000000 c=22.944237
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
2.3 pix Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
2.6 pix fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
2.6 pix fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
Limiting magnitude estimates:
15.4 mag. Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
15.4 mag. Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
15.1 mag. fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
15.1 mag. fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
All-image limiting magnitude estimate: 15.1 (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.vrtnKxgI9f (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=363, passed=5868
Got 5868 stars (including 5502 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
util/solve_plate_with_UCAC5 got 5868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dEe446T9AQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=372, passed=5872
Got 5872 stars (including 5497 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 5872 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ueRWyRtfN3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=418, passed=5319
Got 5319 stars (including 4893 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat
util/solve_plate_with_UCAC5 got 5319 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
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(), 5205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits -region wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.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.G8dw6dDL3z (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=441, passed=5311
Got 5311 stars (including 4863 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat
util/solve_plate_with_UCAC5 got 5311 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5199 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits -region wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
Saving fully-calibrated image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits'
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits'
Preparing the HTML report for the field Vir-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20348.dat to exclusion_list_gaiadr2.txt
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20348_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 20348_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:42:51.32 +14:25:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.527 3741161950722976384 205.71396077119 +14.42643997820 12.3972 11.7454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20350_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 20350_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:43:26.74 +11:06:58.7 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-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat to cache
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Creating symlink local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits exists and is non-empty
wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits exists and is non-empty
wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits exists and is non-empty
wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:52.079 +14:01:57.69
Angular distance between the image centers 0.0557 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:53.815 +14:02:38.36
Angular distance between the image centers 0.0618 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:19:52.079 +14:01:57.69
Second-epoch second image center 13:19:53.815 +14:02:38.36
Angular distance between the image centers 0.01330 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits &> /tmp/tmp.GO38esjbF9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits &> /tmp/tmp.zPI4KezI7J
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits &> /tmp/tmp.tHbfPo2wrT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits &> /tmp/tmp.HCwG88bitn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
The reference image (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits) and catalog (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat) found
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat' -> 'wcsmag.cat'
Read 30168 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 191.7108 to 208.6501 deg, Dec +8.0896 to +19.6104 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 191.7108 to 208.6501 deg, Dec 8.0896 to 19.6104 deg
Loaded 4057 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2777 out of 3023 total matches.
Matched with Tycho-2 3023 out of 30168 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.816035
a=0.000000 b=1.000000 c=22.816035
From vast_summary.log: estimated ref. image limiting mag.: -7.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
2.2 pix Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
2.5 pix fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
2.5 pix fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
Limiting magnitude estimates:
15.6 mag. Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
15.6 mag. Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
15.3 mag. fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
15.3 mag. fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (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.GO38esjbF9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1276, passed=30154
Got 30154 stars (including 28848 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
util/solve_plate_with_UCAC5 got 30154 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 29813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 29814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 29814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zPI4KezI7J (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1283, passed=30242
Got 30242 stars (including 28923 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 30242 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 29812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 29812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 29812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tHbfPo2wrT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1902, passed=24429
Got 24429 stars (including 22497 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat
util/solve_plate_with_UCAC5 got 24429 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
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(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 23872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
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(), 23872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 23872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits -region wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.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.HCwG88bitn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1942, passed=24463
Got 24463 stars (including 22490 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat
util/solve_plate_with_UCAC5 got 24463 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 23882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 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(), 23883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 23883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits -region wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Saving fully-calibrated image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-55-14_20.00sec_-4.90C_LIGHT_0262.fits
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Vir-01-Q2b1x1_044701_TTUQ2b1x1_32284_rIeaYWfX/wcs_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263.fits
Preparing the HTML report for the field Vir-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out11300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52361.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 51834_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 51834_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:02:52.34 +10:11:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52075_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
Preparing report for the candidate 52075_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
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Considering the candidate 52249_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 52249_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:18:50.87 +11:51:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52337_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 52337_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:42:12.01 +10:47:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.483 3726397777304401536 205.55045854362 +10.78798363246 13.8805 13.1893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52344_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 52344_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:10:01.50 +16:10:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52353_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 52353_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:21:49.13 +10:44:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52361_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
Preparing report for the candidate 52361_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52397_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 52397_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:40:23.64 +12:13:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52470_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 52470_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:44:43.37 +10:09:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52604_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 52604_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:47:45.31 +10:41:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 0.743 3727098681607338112 206.93885810629 +10.69814020454 14.6179 14.0320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52633_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 52633_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks
**** FOUND 13:45:10.24 +10:57:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 2.376 3726373347530495232 206.29326074452 +10.95928096503 14.4809 13.5304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52657_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263
The candidate 52657_fd_Vir-01-Q2b1x1_2026-04-10_03-56-07_20.00sec_-4.90C_LIGHT_0263 did not pass the final checks