This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7220,11.47,0.05,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 20260413.2220 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7220,14.10,0.05,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 20260413.2220 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7220,12.86,0.05,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 20260413.2220 12.86CV 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: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461143.72235339 13.04.2026 05:20:01.333 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.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.: -7.63
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15006
Objects passed selection criteria: 14964
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 11598.2
Average stars matched: 11313.5 (97.5449 %)
Memory usage VmPeak: 119760 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 00:22:35 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: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461143.72235339 13.04.2026 05:20:01.333 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 26
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 21 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): 85942
Objects passed selection criteria: 85784
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 70969.8
Average stars matched: 68593.8 (96.6521 %)
Memory usage VmPeak: 1936164 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 00:23:44 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/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.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: 2461143.72156366
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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
Saving wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits to local_wcs_cache/
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
Saving wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits to local_wcs_cache/
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits'
wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:36.282 +06:02:46.60
Angular distance between the image centers 0.0987 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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:33.822 +06:02:21.09
Angular distance between the image centers 0.0864 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 08:34:36.282 +06:02:46.60
Second-epoch second image center 08:34:33.822 +06:02:21.09
Angular distance between the image centers 0.01241 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/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.pHYw2KCMiF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.DqXk4VjeGs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits &> /tmp/tmp.oeoxgWkysC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits &> /tmp/tmp.cG4wgcpwQc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat' -> 'wcsmag.cat'
Read 15650 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.5654 to 136.5445 deg, Dec +0.6765 to +11.2689 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 120.5654 to 136.5445 deg, Dec 0.6765 to 11.2689 deg
Loaded 8720 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): 7106 out of 7589 total matches.
Matched with Tycho-2 7589 out of 15650 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955413
a=0.000000 b=1.000000 c=22.955413
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.3 pix Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.2 pix fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
2.2 pix fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
Limiting magnitude estimates:
15.3 mag. Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.3 mag. Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
14.6 mag. fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
14.5 mag. fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.6 (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.pHYw2KCMiF (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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1186, passed=15650
Got 15650 stars (including 14444 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 15650 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 15104 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 15107 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 15107 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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.DqXk4VjeGs (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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1188, passed=15565
Got 15565 stars (including 14349 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 15565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15149 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 15147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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.oeoxgWkysC (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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=514, passed=8078
Got 8078 stars (including 7558 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat
util/solve_plate_with_UCAC5 got 8078 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 7684 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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 7686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 7686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits -region wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.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.cG4wgcpwQc (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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=492, passed=7406
Got 7406 stars (including 6903 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat
util/solve_plate_with_UCAC5 got 7406 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 7136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 7134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 7134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits -region wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
Saving fully-calibrated image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits'
Preparing the HTML report for the field Hya-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20923.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20814_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 20814_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:06:01.70 +07:24:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.37, MAG_FAINT_SEARCH_LIMIT=11.35)GAIADR2_OUTPUT=# 0.678 584211557660771456 136.50726332291 +07.40486530794 9.9626 9.1200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20853_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 20853_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:06:06.29 +09:34:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 0.883 591331170328265856 136.52600473767 +09.57352565897 10.8041 10.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20923_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
Preparing report for the candidate 20923_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Hya-01-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 ####
08:58:48.72 +09:45:21.8
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/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Creating symlink local_wcs_cache/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits exists and is non-empty
wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:36.282 +06:02:46.60
Angular distance between the image centers 0.0987 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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:33.822 +06:02:21.09
Angular distance between the image centers 0.0864 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 08:34:36.282 +06:02:46.60
Second-epoch second image center 08:34:33.822 +06:02:21.09
Angular distance between the image centers 0.01241 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/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.FJGePCeD9q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.KexOIOSkXs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits &> /tmp/tmp.VjBOae0DBT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits &> /tmp/tmp.FCDNtBuWzq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat' -> 'wcsmag.cat'
Read 90472 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.5655 to 136.5508 deg, Dec +0.6702 to +11.2724 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 120.5655 to 136.5508 deg, Dec 0.6702 to 11.2724 deg
Loaded 8738 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): 6435 out of 7690 total matches.
Matched with Tycho-2 7690 out of 90472 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.847783
a=0.000000 b=1.000000 c=22.847783
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.1 pix Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.0 pix fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
2.2 pix fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
Limiting magnitude estimates:
15.5 mag. Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.5 mag. Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
14.8 mag. fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
14.7 mag. fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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.FJGePCeD9q (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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6373, passed=90453
Got 90453 stars (including 83928 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 90453 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 88129 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 88126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 88125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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.KexOIOSkXs (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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=6475, passed=90928
Got 90928 stars (including 84300 good ones) from the SExtractor catalog wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 90928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 88620 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 88620 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 88620 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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.VjBOae0DBT (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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2941, passed=53817
Got 53817 stars (including 50775 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat
util/solve_plate_with_UCAC5 got 53817 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 51384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 51381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 51381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits -region wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.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.FCDNtBuWzq (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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
Checking if the catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat corresponding to the image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
WCS catalog name: wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2655, passed=50733
Got 50733 stars (including 47973 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat
util/solve_plate_with_UCAC5 got 50733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 48717 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 48717 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 48717 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits -region wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.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_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Saving fully-calibrated image wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/wcs_Hya-01-Q1b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-18-53_20.00sec_-5.00C_LIGHTs_0042.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.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_2026-04-13_CI_Hya-01-Q1b1x1_002058_TTUQ1b1x1_3274_QJvlrGdU/wcs_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043.fits
Preparing the HTML report for the field Hya-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out107250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out108775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52873.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107239_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107239_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:38:12.50 +03:34:27.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107250_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107250_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:38:29.76 +03:24:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.777 3080115081700107264 129.62423714695 +03.40596076813 13.8938 13.4208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107251_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107251_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:00:43.81 +00:57:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.876 576582218274157440 135.18268273331 +00.95878162603 13.6824 13.2413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107252_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107252_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:58:28.84 +02:32:03.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107263_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107263_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:03:29.83 +04:12:46.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107327_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107327_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:06:01.70 +07:24:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.36, MAG_FAINT_SEARCH_LIMIT=11.34)GAIADR2_OUTPUT=# 0.678 584211557660771456 136.50726332291 +07.40486530794 9.9626 9.1200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107365_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107365_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:06:06.30 +09:34:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 1.062 591331170328265856 136.52600473767 +09.57352565897 10.8041 10.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107442_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107442_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:58:48.71 +09:45:21.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107762_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107762_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:37:49.18 +05:42:47.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107804_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107804_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:06:34.92 +09:28:41.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107837_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107837_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:41:12.39 +00:56:21.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107879_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107879_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 09:06:05.06 +09:00:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 0.392 591155656489344128 136.52118084372 +09.01235636637 12.9972 12.5097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107887_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 107887_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:52:14.69 +04:53:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.845 581870113289750144 133.06101998362 +04.89441880450 13.0179 12.5406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108566_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 108566_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:49:29.97 +00:53:56.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108775_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
Preparing report for the candidate 108775_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109187_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043
The candidate 109187_fd_Hya-01-Q1b1x1_2026-04-13_00-20-01_20.00sec_-5.00C_LIGHTs_0043 did not pass the final checks