This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN
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,2461139.7312,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2312 13.18CV 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
KS Hya,2461139.7312,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KS Hya 20260409.2312 12.46CV 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
FT Hya,2461139.7312,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FT Hya 20260409.2312 11.75CV 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: 2461118.86466318 19.03.2026 08:44:56.899 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
First image: 2461118.86466318 19.03.2026 08:44:56.899 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Last image: 2461139.73158286 09.04.2026 05:33:18.759 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.22
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): 5310
Objects passed selection criteria: 5301
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 4417.5
Average stars matched: 4332.75 (98.0815 %)
Memory usage VmPeak: 111844 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:39:48 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: 2461118.86466318 19.03.2026 08:44:56.899 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
First image: 2461118.86466318 19.03.2026 08:44:56.899 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Last image: 2461139.73158286 09.04.2026 05:33:18.759 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.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.: -7.88
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: 11 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): 35233
Objects passed selection criteria: 35176
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 31745.5
Average stars matched: 30801.5 (97.0264 %)
Memory usage VmPeak: 140732 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:40:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
SExtractor catalog cache: saved Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat to cache
SExtractor catalog cache: saved Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461139.73080163
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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits exists and is non-empty
Saving wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits to local_wcs_cache/
'wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits' -> 'local_wcs_cache/wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits'
wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits exists and is non-empty
Saving wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits to local_wcs_cache/
'wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits' -> 'local_wcs_cache/wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits'
wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits exists and is non-empty
Saving wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits to local_wcs_cache/
'wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits' -> 'local_wcs_cache/wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits'
wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits exists and is non-empty
Saving wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits to local_wcs_cache/
'wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits' -> 'local_wcs_cache/wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:24:09.002 -25:59:19.42
Second-epoch image center 14:24:00.327 -26:00:25.05
Angular distance between the image centers 0.0373 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 14:24:09.002 -25:59:19.42
Second-epoch image center 14:24:03.016 -26:00:01.32
Angular distance between the image centers 0.0253 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 14:24:00.327 -26:00:25.05
Second-epoch second image center 14:24:03.016 -26:00:01.32
Angular distance between the image centers 0.01204 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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits &> /tmp/tmp.jF5Uv0Jdvb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits &> /tmp/tmp.EWgebU5MDW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits &> /tmp/tmp.7f8jtyvv2H
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits &> /tmp/tmp.Y28g6SUxXq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
Found non-empty wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
The reference image (wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits) and catalog (wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat) found
'wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat' -> 'wcsmag.cat'
Read 7306 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 206.8784 to 225.0225 deg, Dec -31.2717 to -20.4641 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 206.8784 to 225.0225 deg, Dec -31.2717 to -20.4641 deg
Loaded 7631 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): 5349 out of 5503 total matches.
Matched with Tycho-2 5503 out of 7306 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.777156
a=0.000000 b=1.000000 c=22.777156
From vast_summary.log: estimated ref. image limiting mag.: -8.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
2.4 pix Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
2.5 pix fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
2.5 pix fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
Limiting magnitude estimates:
14.6 mag. Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
14.6 mag. Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
13.9 mag. fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
13.9 mag. fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.1 (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.jF5Uv0Jdvb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits' -> 'wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS_IMAGE_NAME=wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS-calibrated image found: wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Checking if the catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits alredy exist and is non-empty...
Catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS catalog name: wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=484, passed=7306
Got 7306 stars (including 6818 good ones) from the SExtractor catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
util/solve_plate_with_UCAC5 got 7306 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 7146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 7146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 7146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits -region wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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.EWgebU5MDW (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits' -> 'wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS-calibrated image found: wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Checking if the catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS catalog name: wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=477, passed=7284
Got 7284 stars (including 6803 good ones) from the SExtractor catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 7284 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 7115 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 7113 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 7113 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits -region wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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.7f8jtyvv2H (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
WCS-calibrated image found: wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
Checking if the catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat corresponding to the image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat corresponding to the image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
WCS catalog name: wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=319, passed=4387
Got 4387 stars (including 4067 good ones) from the SExtractor catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 4387 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits -region wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.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.Y28g6SUxXq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
Checking if the catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat corresponding to the image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat corresponding to the image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
WCS catalog name: wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=326, passed=4404
Got 4404 stars (including 4077 good ones) from the SExtractor catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 4404 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4340 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4340 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 4340 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits -region wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits'
Saving fully-calibrated image wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits'
Saving fully-calibrated image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits'
Saving fully-calibrated image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits'
Preparing the HTML report for the field Hya-14-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Hya-14-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
SExtractor catalog cache: saved Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat to cache
SExtractor catalog cache: saved Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Creating symlink local_wcs_cache/wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits exists and is non-empty
wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits exists and is non-empty
wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits exists and is non-empty
wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:24:09.002 -25:59:19.42
Second-epoch image center 14:24:00.327 -26:00:25.05
Angular distance between the image centers 0.0373 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 14:24:09.002 -25:59:19.42
Second-epoch image center 14:24:03.016 -26:00:01.32
Angular distance between the image centers 0.0253 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 14:24:00.327 -26:00:25.05
Second-epoch second image center 14:24:03.016 -26:00:01.32
Angular distance between the image centers 0.01204 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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits &> /tmp/tmp.Ns4eTZNvNf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits &> /tmp/tmp.MmF1357340
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits &> /tmp/tmp.bw5NWPWec1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits &> /tmp/tmp.GcR7Br8Uok
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
Found non-empty wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits and wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
The reference image (wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits) and catalog (wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat) found
'wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat' -> 'wcsmag.cat'
Read 48077 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 206.8452 to 225.0425 deg, Dec -31.2754 to -20.4430 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 206.8452 to 225.0425 deg, Dec -31.2754 to -20.4430 deg
Loaded 7679 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): 5937 out of 6447 total matches.
Matched with Tycho-2 6447 out of 48077 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.585793
a=0.000000 b=1.000000 c=22.585793
From vast_summary.log: estimated ref. image limiting mag.: -7.88
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.71
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.71
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
2.3 pix Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
2.1 pix fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
2.1 pix fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
Limiting magnitude estimates:
14.7 mag. Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
14.7 mag. Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
14.1 mag. fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
14.1 mag. fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Ns4eTZNvNf (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits' -> 'wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS_IMAGE_NAME=wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS-calibrated image found: wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Checking if the catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits alredy exist and is non-empty...
Catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat corresponding to the image wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
WCS catalog name: wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2143, passed=48070
Got 48070 stars (including 45854 good ones) from the SExtractor catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat
util/solve_plate_with_UCAC5 got 48070 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 46948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 46945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 46945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits -region wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.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.MmF1357340 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits' -> 'wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS-calibrated image found: wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Checking if the catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat corresponding to the image wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
WCS catalog name: wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2237, passed=47983
Got 47983 stars (including 45685 good ones) from the SExtractor catalog wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 47983 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 46984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 46987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 46987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits -region wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.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.bw5NWPWec1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
WCS-calibrated image found: wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
Checking if the catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat corresponding to the image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat corresponding to the image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
WCS catalog name: wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1136, passed=32851
Got 32851 stars (including 31674 good ones) from the SExtractor catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 32851 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 32291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 32292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 32292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits -region wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.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.GcR7Br8Uok (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
Checking if the catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat corresponding to the image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat corresponding to the image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
WCS catalog name: wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1175, passed=32841
Got 32841 stars (including 31626 good ones) from the SExtractor catalog wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 32841 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 32292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 32292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 32292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits -region wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.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-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/wcs_Hya-14-Q2b1x1_2026-03-19_03-44-56_20.00sec_-15.00C_LIGHT_0106.fits
Saving fully-calibrated image wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/wcs_Hya-14-Q2b1x1_2026-03-19_03-45-42_20.00sec_-14.90C_LIGHT_0107.fits
Saving fully-calibrated image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-32-11_20.00sec_-4.90C_LIGHT_0191.fits
Saving fully-calibrated image wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Hya-14-Q2b1x1_013737_TTUQ2b1x1_303_1MGv8LTN/wcs_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192.fits
Preparing the HTML report for the field Hya-14-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out22522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53387.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
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Considering the candidate 53080_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53080_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:08:22.54 -29:01:16.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 53082_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53082_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:13:57.01 -24:05:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53084_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53084_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:30:41.42 -23:53:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53086_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53086_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 53087_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53087_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:38:48.73 -24:13:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.993 6278054301877158144 219.70295509987 -24.21768094271 12.2912 11.5879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53088_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53088_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:03:39.44 -24:06:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53123_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53123_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:44:00.96 -27:21:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 0.123 6222515289500583040 221.00402694741 -27.36225320083 10.5501 9.8169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.123#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53137_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53137_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:32:17.37 -24:02:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 1.013 6272301901855482368 218.07232738180 -24.03905568340 11.2581 10.8154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53186_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53186_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:40:52.13 -26:25:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 1.085 6223555668018224000 220.21689710789 -26.42544835150 11.8857 11.3640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53281_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53281_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:39:05.24 -27:20:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 1.166 6222645272390895744 219.77150436732 -27.34330455234 12.6839 12.2066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53341_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53341_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:03:20.14 -24:48:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53349_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53349_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:41:59.16 -29:21:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 0.691 6218851240015650304 220.49671985991 -29.36476621265 12.8456 12.4097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53370_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53370_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:42:07.28 -28:56:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53387_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
Preparing report for the candidate 53387_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
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Considering the candidate 53404_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53404_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:09:51.09 -27:23:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53425_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53425_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:43:26.94 -24:27:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53437_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53437_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:34:39.79 -23:33:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.516 6278327019417069952 218.66503420767 -23.56035706464 13.5477 12.9424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53441_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53441_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:09:22.68 -25:03:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53443_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53443_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:04:44.16 -27:28:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.816 6270493205227589888 211.18425435855 -27.47557543938 13.1429 12.5133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53446_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53446_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:28:58.78 -25:19:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53477_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53477_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:07:55.44 -22:10:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53517_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53517_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:20:20.39 -25:08:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53600_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 53600_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks
**** FOUND 14:41:06.08 -23:21:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.839 6278213288683200512 220.27484850821 -23.35430608789 14.4575 13.8759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22522_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
Preparing report for the candidate 22522_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
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Considering the candidate 27046_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
Preparing report for the candidate 27046_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
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Considering the candidate 08608_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192
The candidate 08608_fd_Hya-14-Q2b1x1_2026-04-09_00-33-18_20.00sec_-4.90C_LIGHT_0192 did not pass the final checks