This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5456459704201088768,2461136.6498,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5456459704201088768 20260406.1498 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1498* 10 18 29.92 -29 03 25.8 13.2 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.6498,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.1498 13.19CV 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: 2461121.72219900 22.03.2026 05:19:47.994 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
First image: 2461121.72219900 22.03.2026 05:19:47.994 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Last image: 2461136.65009653 06.04.2026 03:35:58.340 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.09
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: 5 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): 7822
Objects passed selection criteria: 7814
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 7300.25
Average stars matched: 7163 (98.1199 %)
Memory usage VmPeak: 113672 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 22:41:13 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: 2461121.72219900 22.03.2026 05:19:47.994 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
First image: 2461121.72219900 22.03.2026 05:19:47.994 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Last image: 2461136.65009653 06.04.2026 03:35:58.340 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 43
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.86
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: 22 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): 45147
Objects passed selection criteria: 45103
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 41415.8
Average stars matched: 40142.8 (96.9263 %)
Memory usage VmPeak: 147416 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 22:42:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat to cache
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.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: 2461136.64944124
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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
Saving wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits to local_wcs_cache/
'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits' -> 'local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits'
wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
Saving wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits to local_wcs_cache/
'wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits'
wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits exists and is non-empty
Saving wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits to local_wcs_cache/
'wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits' -> 'local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits'
wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits exists and is non-empty
Saving wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits to local_wcs_cache/
'wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits' -> 'local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.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 10:33:35.280 -26:00:04.03
Second-epoch image center 10:33:33.222 -25:59:58.53
Angular distance between the image centers 0.0079 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 10:33:35.280 -26:00:04.03
Second-epoch image center 10:33:36.062 -26:00:13.08
Angular distance between the image centers 0.0039 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 10:33:33.222 -25:59:58.53
Second-epoch second image center 10:33:36.062 -26:00:13.08
Angular distance between the image centers 0.01138 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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.3Ai99cNJuX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.1Q3YuOyNYX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits &> /tmp/tmp.pV3MKH8bAm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits &> /tmp/tmp.9yzKZAaf5v
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
Found non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
The reference image (wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits) and catalog (wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat) found
'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat' -> 'wcsmag.cat'
Read 9188 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.1995 to 167.3695 deg, Dec -31.3041 to -20.4278 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 149.1995 to 167.3695 deg, Dec -31.3041 to -20.4278 deg
Loaded 8646 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): 6476 out of 6648 total matches.
Matched with Tycho-2 6648 out of 9188 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.827572
a=0.000000 b=1.000000 c=22.827572
From vast_summary.log: estimated ref. image limiting mag.: -8.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.74
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.74
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
2.3 pix Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
3.2 pix fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
3.2 pix fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
Limiting magnitude estimates:
14.7 mag. Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
14.8 mag. Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
14.3 mag. fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
14.3 mag. fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.7 (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.3Ai99cNJuX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits' -> 'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=502, passed=9188
Got 9188 stars (including 8670 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 9188 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.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.1Q3YuOyNYX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.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-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=513, passed=9186
Got 9186 stars (including 8663 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 9186 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 8987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 8986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 8986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.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.pV3MKH8bAm (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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=510, passed=7548
Got 7548 stars (including 7027 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat
util/solve_plate_with_UCAC5 got 7548 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 7381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 7381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 7381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits -region wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.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.9yzKZAaf5v (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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=527, passed=7576
Got 7576 stars (including 7044 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat
util/solve_plate_with_UCAC5 got 7576 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 7397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 7396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 7396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
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-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits -region wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits'
Saving fully-calibrated image wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits'
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits'
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits'
Preparing the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat to cache
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Creating symlink local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits exists and is non-empty
wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.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 10:33:35.280 -26:00:04.03
Second-epoch image center 10:33:33.222 -25:59:58.53
Angular distance between the image centers 0.0079 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 10:33:35.280 -26:00:04.03
Second-epoch image center 10:33:36.062 -26:00:13.08
Angular distance between the image centers 0.0039 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 10:33:33.222 -25:59:58.53
Second-epoch second image center 10:33:36.062 -26:00:13.08
Angular distance between the image centers 0.01138 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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.q1c13J3Nio
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.7OHl95NegH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits &> /tmp/tmp.lyEsMDt5h6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits &> /tmp/tmp.sF7O79rTwn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
Found non-empty wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
The reference image (wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits) and catalog (wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat) found
'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat' -> 'wcsmag.cat'
Read 52516 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 149.1799 to 167.4334 deg, Dec -31.3047 to -20.4069 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 149.1799 to 167.4334 deg, Dec -31.3047 to -20.4069 deg
Loaded 8722 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): 6662 out of 7301 total matches.
Matched with Tycho-2 7301 out of 52516 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.700451
a=0.000000 b=1.000000 c=22.700451
From vast_summary.log: estimated ref. image limiting mag.: -7.86
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.84
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
2.4 pix Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
2.9 pix fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
2.9 pix fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
Limiting magnitude estimates:
14.8 mag. Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
14.9 mag. Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
14.5 mag. fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
14.5 mag. fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 13.8 (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.q1c13J3Nio (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits' -> 'wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2425, passed=52512
Got 52512 stars (including 49995 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 52512 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 51223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 51223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 51224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.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.7OHl95NegH (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.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-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=2429, passed=53236
Got 53236 stars (including 50714 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 53236 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 51985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 51984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 51983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.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.lyEsMDt5h6 (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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=3020, passed=38847
Got 38847 stars (including 35794 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat
util/solve_plate_with_UCAC5 got 38847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
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...
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 38110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 38109 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
WARNING: Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 38109 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits -region wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.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.sF7O79rTwn (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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS-calibrated image found: wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
Checking if the catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS catalog name: wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=3030, passed=39128
Got 39128 stars (including 36063 good ones) from the SExtractor catalog wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat
util/solve_plate_with_UCAC5 got 39128 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
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...
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 38307 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 38307 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 38307 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits -region wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.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-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/wcs_Hya-10-Q2b1x1_2026-03-22_00-19-47_20.00sec_-14.90C_LIGHT_0053.fits
Saving fully-calibrated image wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/wcs_Hya-10-Q2b1x1_2026-03-22_00-20-36_20.00sec_-15.00C_LIGHT_0054.fits
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-01_20.00sec_-4.90C_LIGHT_0082.fits
Saving fully-calibrated image wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.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_2026-04-05_CI_Hya-10-Q2b1x1_223641_TTUQ2b1x1_9752_wFHB0CCl/wcs_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083.fits
Preparing the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out66489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out66515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66828.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 66489_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 66489_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:34:37.56 -22:16:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 0.559 5474819418080843008 158.65666315045 -22.27698125311 14.5553 14.1105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66500_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 66500_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:20:43.87 -25:48:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.361 5472102043812323328 155.18331568182 -25.81265566469 13.7825 13.0873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66509_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 66509_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:44:27.02 -26:23:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66515_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 66515_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
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Considering the candidate 66516_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 66516_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:31:02.54 -26:44:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.814 5469100342708939904 157.76070332518 -26.73768965972 13.1753 12.6290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66522_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 66522_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:29:19.49 -28:47:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.608 5467695407366661888 157.33127420922 -28.78711893312 12.8735 12.1660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66779_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 66779_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:23:33.17 -23:27:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66828_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 66828_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
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Considering the candidate 66902_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 66902_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:32:26.45 -24:31:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.063 5471139077784569344 158.11062731274 -24.53209983415 13.6009 12.9404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66931_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 66931_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:14:27.04 -24:12:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66974_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 66974_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:25:37.97 -22:31:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 2.398 5475317874805139968 156.40760887923 -22.52117597557 14.2442 13.8309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67006_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 67006_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:21:13.10 -22:33:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.810 5475537227374464256 155.30477389970 -22.56238754262 14.2947 13.7484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67015_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 67015_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:07:07.09 -22:47:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.084 5665983086665802496 151.77922795215 -22.79872123188 14.3982 13.7902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67017_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 67017_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:25:04.65 -23:12:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.865 5474503136689132544 156.26914142544 -23.21002466866 14.6592 14.2000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67030_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 67030_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 10:20:04.68 -28:30:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.627 5462542924080126208 155.01924357023 -28.50038594424 14.2310 13.6121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67060_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083
The candidate 67060_fd_Hya-10-Q2b1x1_2026-04-05_22-35-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks