This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN
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
BG Hya,2461144.6944,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BG Hya 20260414.1944 12.09CV 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
BF Hya,2461144.6944,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BF Hya 20260414.1944 12.21CV 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: 2461121.72798492 22.03.2026 05:28:07.897 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
First image: 2461121.72798492 22.03.2026 05:28:07.897 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
Last image: 2461144.69481037 14.04.2026 04:40:21.616 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.40
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): 6751
Objects passed selection criteria: 6740
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: 5848.5
Average stars matched: 5720.25 (97.8071 %)
Memory usage VmPeak: 112680 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 23:46:16 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: 2461121.72798492 22.03.2026 05:28:07.897 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
First image: 2461121.72798492 22.03.2026 05:28:07.897 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
Last image: 2461144.69481037 14.04.2026 04:40:21.616 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 31
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.18
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: 12 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): 39550
Objects passed selection criteria: 39522
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 34460
Average stars matched: 33636.5 (97.6103 %)
Memory usage VmPeak: 141792 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 23:47:12 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
SExtractor catalog cache: saved Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat to cache
SExtractor catalog cache: saved Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.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: 2461144.69399071
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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits exists and is non-empty
Saving wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits to local_wcs_cache/
'wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits' -> 'local_wcs_cache/wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits'
wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits exists and is non-empty
Saving wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits to local_wcs_cache/
'wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits'
wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits exists and is non-empty
Saving wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits to local_wcs_cache/
'wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits' -> 'local_wcs_cache/wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits'
wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits exists and is non-empty
Saving wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits to local_wcs_cache/
'wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits' -> 'local_wcs_cache/wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:28:42.244 -33:59:56.33
Second-epoch image center 11:28:34.952 -34:01:21.59
Angular distance between the image centers 0.0346 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 11:28:42.244 -33:59:56.33
Second-epoch image center 11:28:32.330 -34:01:33.72
Angular distance between the image centers 0.0436 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 11:28:34.952 -34:01:21.59
Second-epoch second image center 11:28:32.330 -34:01:33.72
Angular distance between the image centers 0.00966 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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits &> /tmp/tmp.XGEKsLKlOb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits &> /tmp/tmp.wN7RSIkzCE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits &> /tmp/tmp.0YE7F4a6sL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits &> /tmp/tmp.tMG1ui4IDW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat
Found non-empty wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat
The reference image (wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits) and catalog (wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat) found
'wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat' -> 'wcsmag.cat'
Read 7026 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 162.0209 to 181.9887 deg, Dec -39.3258 to -28.3161 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 162.0209 to 181.9887 deg, Dec -39.3258 to -28.3161 deg
Loaded 9693 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): 5749 out of 5869 total matches.
Matched with Tycho-2 5869 out of 7026 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.719786
a=0.000000 b=1.000000 c=22.719786
From vast_summary.log: estimated ref. image limiting mag.: -8.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
2.4 pix Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
3.1 pix fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
3.1 pix fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
Limiting magnitude estimates:
14.3 mag. Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
14.3 mag. Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
13.6 mag. fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
13.7 mag. fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.0 (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.XGEKsLKlOb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits' -> 'wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
Checking if the catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
WCS catalog name: wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=417, passed=7026
Got 7026 stars (including 6594 good ones) from the SExtractor catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 7026 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 6843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits -region wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.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.wN7RSIkzCE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.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-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits' -> 'wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
Checking if the catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
WCS catalog name: wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=412, passed=7121
Got 7121 stars (including 6698 good ones) from the SExtractor catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 7121 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.3)
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: 967 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 6947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 253 to 310 (Dec -39.3 to -28.3)
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: 967 matched stars entering correct_measured_positions(), 6947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 6947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits -region wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.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.0YE7F4a6sL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
WCS_IMAGE_NAME=wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
WCS-calibrated image found: wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
Checking if the catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat corresponding to the image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat corresponding to the image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
WCS catalog name: wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=239, passed=4684
Got 4684 stars (including 4441 good ones) from the SExtractor catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat
util/solve_plate_with_UCAC5 got 4684 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.7'
Seting catalog search parameters based on the expected field of view 940.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013065 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010452 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 4588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 4586 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 4586 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits -region wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.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.tMG1ui4IDW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
WCS_IMAGE_NAME=wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
WCS-calibrated image found: wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
Checking if the catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat corresponding to the image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat corresponding to the image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
WCS catalog name: wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=247, passed=4709
Got 4709 stars (including 4457 good ones) from the SExtractor catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat
util/solve_plate_with_UCAC5 got 4709 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 4615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 966 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(), 4614 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 4622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 964 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits -region wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits'
Saving fully-calibrated image wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits'
Saving fully-calibrated image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits'
Saving fully-calibrated image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits'
Preparing the HTML report for the field Hya-15-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03818_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 03818_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:09:16.77 -33:37:10.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Hya-15-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
SExtractor catalog cache: saved Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat to cache
SExtractor catalog cache: saved Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
Creating symlink local_wcs_cache/wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits exists and is non-empty
wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits exists and is non-empty
wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits exists and is non-empty
wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:28:42.244 -33:59:56.33
Second-epoch image center 11:28:34.952 -34:01:21.59
Angular distance between the image centers 0.0346 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 11:28:42.244 -33:59:56.33
Second-epoch image center 11:28:32.330 -34:01:33.72
Angular distance between the image centers 0.0436 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 11:28:34.952 -34:01:21.59
Second-epoch second image center 11:28:32.330 -34:01:33.72
Angular distance between the image centers 0.00966 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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits &> /tmp/tmp.fnJLs5XVUj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits &> /tmp/tmp.zq8K7oiwhd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits &> /tmp/tmp.iIp0pHPXR1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits &> /tmp/tmp.mmtXZkK2Rl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat
Found non-empty wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat
The reference image (wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits) and catalog (wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat) found
'wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat' -> 'wcsmag.cat'
Read 42959 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 161.9359 to 182.0452 deg, Dec -39.3258 to -28.2459 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 161.9359 to 182.0452 deg, Dec -39.3258 to -28.2459 deg
Loaded 9810 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): 7530 out of 7992 total matches.
Matched with Tycho-2 7992 out of 42959 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.569555
a=0.000000 b=1.000000 c=22.569555
From vast_summary.log: estimated ref. image limiting mag.: -8.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.39
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 24 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
2.5 pix Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
2.9 pix fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
2.8 pix fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
Limiting magnitude estimates:
14.4 mag. Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
14.4 mag. Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
13.8 mag. fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
13.8 mag. fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (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.fnJLs5XVUj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits' -> 'wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
Checking if the catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
WCS catalog name: wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1578, passed=42957
Got 42957 stars (including 41309 good ones) from the SExtractor catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 42957 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 971 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(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 41897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 971 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(), 41895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 41895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits -region wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.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.zq8K7oiwhd (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.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-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits' -> 'wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
Checking if the catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
WCS catalog name: wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1548, passed=41735
Got 41735 stars (including 40124 good ones) from the SExtractor catalog wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 41735 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 40598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 40597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 40597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits -region wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.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.iIp0pHPXR1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
WCS_IMAGE_NAME=wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
WCS-calibrated image found: wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
Checking if the catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat corresponding to the image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat corresponding to the image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
WCS catalog name: wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=828, passed=26795
Got 26795 stars (including 25935 good ones) from the SExtractor catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat
util/solve_plate_with_UCAC5 got 26795 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.7'
Seting catalog search parameters based on the expected field of view 940.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013065 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010452 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 312 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 26303 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 252 to 312 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 26303 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 26304 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits -region wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.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.mmtXZkK2Rl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
WCS_IMAGE_NAME=wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
WCS-calibrated image found: wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
Checking if the catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat corresponding to the image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat corresponding to the image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
WCS catalog name: wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=823, passed=27282
Got 27282 stars (including 26426 good ones) from the SExtractor catalog wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat
util/solve_plate_with_UCAC5 got 27282 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 966 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(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 26738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 966 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(), 26738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 26738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits -region wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.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-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/wcs_Hya-15-Q1b1x1_2026-03-22_00-28-07_20.00sec_-15.00C_LIGHT_0061.fits
Saving fully-calibrated image wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/wcs_Hya-15-Q1b1x1_2026-03-22_00-29-04_20.00sec_-15.00C_LIGHT_0062.fits
Saving fully-calibrated image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-39-10_20.00sec_-4.90C_LIGHTs_0129.fits
Saving fully-calibrated image wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-15-Q1b1x1_234116_TTUQ1b1x1_12154_PtAIkJuN/wcs_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130.fits
Preparing the HTML report for the field Hya-15-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out25128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31359.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 52679_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 52679_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:30:54.21 -37:53:42.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)
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Considering the candidate 52682_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 52682_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:38:04.94 -30:00:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52683_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 52683_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:58:05.64 -31:47:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52863_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 52863_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 12:04:36.48 -31:10:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52881_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 52881_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:08:44.43 -29:44:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52941_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 52941_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 10:59:08.00 -34:20:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52942_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 52942_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 10:58:11.12 -31:33:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.237 5450476333721752832 164.54589041097 -31.55456180933 12.9910 12.3384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52979_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 52979_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:13:53.03 -30:04:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.693 5452359487902458624 168.47178762923 -30.07023836702 13.4670 12.9125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52988_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 52988_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:55:32.64 -31:13:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52997_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 52997_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:26:58.65 -29:56:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.357 3482221911501341056 171.74362421060 -29.94799053990 13.3048 12.6354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53029_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 53029_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:00:16.25 -28:26:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53042_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 53042_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:27:42.02 -32:09:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53055_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 53055_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:45:12.86 -31:09:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53085_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 53085_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 12:04:47.20 -30:30:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53095_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 53095_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:37:23.23 -29:38:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53101_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 53101_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:52:02.03 -31:54:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53111_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 53111_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:48:46.08 -29:32:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.233 3480747638206993664 177.19167569839 -29.54694401434 13.8893 13.4312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53120_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 53120_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:55:17.33 -29:40:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53124_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 53124_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:52:30.50 -31:48:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.593 3479181040296047744 178.12716829078 -31.81267455761 13.9185 13.4159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53126_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 53126_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:40:23.31 -33:22:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.603 3477625192686127360 175.09663676214 -33.37381766295 14.1850 13.6708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22240_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 22240_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks
**** FOUND 11:09:16.77 -33:37:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11367_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130
The candidate 11367_fd_Hya-15-Q1b1x1_2026-04-13_23-40-21_20.00sec_-4.90C_LIGHTs_0130 did not pass the final checks