This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.2079* 09 31 52.80 +09 09 46.8 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7079,12.86,0.05,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 20260413.2079 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7079,14.11,0.05,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 20260413.2079 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.7079,14.70,0.05,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 20260413.2079 14.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
First image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Last image: 2461143.70829062 13.04.2026 04:59:46.310 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8728
Objects passed selection criteria: 8691
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 6573.5
Average stars matched: 6071.75 (92.3671 %)
Memory usage VmPeak: 113716 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 00:02:02 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
First image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Last image: 2461143.70829062 13.04.2026 04:59:46.310 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 64
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 19 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): 49021
Objects passed selection criteria: 48883
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 39051.8
Average stars matched: 36050 (92.3134 %)
Memory usage VmPeak: 145264 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 00:03:00 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461143.70747310
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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits'
wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:48.075 +05:59:40.24
Angular distance between the image centers 0.0219 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 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:48.874 +06:00:03.14
Angular distance between the image centers 0.0243 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 09:25:48.075 +05:59:40.24
Second-epoch second image center 09:25:48.874 +06:00:03.14
Angular distance between the image centers 0.00717 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits &> /tmp/tmp.2iYEuUCKr0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits &> /tmp/tmp.eFvywOt1Jd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits &> /tmp/tmp.T0SEP6dKSB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits &> /tmp/tmp.ttI28ukEFt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat' -> 'wcsmag.cat'
Read 9705 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.2099 to 149.7640 deg, Dec +0.1004 to +11.7220 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 133.2099 to 149.7640 deg, Dec 0.1004 to 11.7220 deg
Loaded 6611 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): 4811 out of 5047 total matches.
Matched with Tycho-2 5047 out of 9705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.925124
a=0.000000 b=1.000000 c=22.925124
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
2.5 pix Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
2.6 pix fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
2.6 pix fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
Limiting magnitude estimates:
15.3 mag. Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
15.3 mag. Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
14.9 mag. fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
14.9 mag. fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2iYEuUCKr0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=629, passed=9705
Got 9705 stars (including 9071 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 9705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 9526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 9526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 9526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eFvywOt1Jd (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=616, passed=9704
Got 9704 stars (including 9075 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 9704 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 9534 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 9536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 9537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 937 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.T0SEP6dKSB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=434, passed=7818
Got 7818 stars (including 7377 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat
util/solve_plate_with_UCAC5 got 7818 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 7606 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 7602 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 7602 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 937 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.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.ttI28ukEFt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=419, passed=7687
Got 7687 stars (including 7257 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat
util/solve_plate_with_UCAC5 got 7687 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 7502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 7501 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 7501 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 936 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits'
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20390_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 20390_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:42:41.75 +08:07:57.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21736_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 21736_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:10:19.60 +04:55:31.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Hya-02-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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits exists and is non-empty
wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:48.075 +05:59:40.24
Angular distance between the image centers 0.0219 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 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:48.874 +06:00:03.14
Angular distance between the image centers 0.0243 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 09:25:48.075 +05:59:40.24
Second-epoch second image center 09:25:48.874 +06:00:03.14
Angular distance between the image centers 0.00717 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits &> /tmp/tmp.pBo35m7Uyf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits &> /tmp/tmp.rHyfVx2Nk9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits &> /tmp/tmp.WNlQo2YBFl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits &> /tmp/tmp.2w4i59QH2H
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat' -> 'wcsmag.cat'
Read 52265 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.1873 to 149.7640 deg, Dec +0.0999 to +11.7791 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 133.1873 to 149.7640 deg, Dec 0.0999 to 11.7791 deg
Loaded 6657 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): 4491 out of 5088 total matches.
Matched with Tycho-2 5088 out of 52265 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.799339
a=0.000000 b=1.000000 c=22.799339
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 39 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
2.3 pix Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
2.3 pix fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
2.3 pix fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
Limiting magnitude estimates:
15.4 mag. Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
15.4 mag. Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
15.2 mag. fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
15.1 mag. fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.pBo35m7Uyf (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=3222, passed=52238
Got 52238 stars (including 48939 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 52238 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 51515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 51515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 51515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rHyfVx2Nk9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=3213, passed=52136
Got 52136 stars (including 48850 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 52136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 51370 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 51371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 51371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WNlQo2YBFl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2283, passed=43383
Got 43383 stars (including 41051 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat
util/solve_plate_with_UCAC5 got 43383 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 42427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 42431 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 42432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.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.2w4i59QH2H (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2268, passed=42926
Got 42926 stars (including 40601 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat
util/solve_plate_with_UCAC5 got 42926 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 42051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 42049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 42048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits -region wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-58-35_20.00sec_-4.90C_LIGHT_0366.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Hya-02-Q2b1x1_000035_TTUQ2b1x1_28508_d4qboUst/wcs_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367.fits
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out65379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65395.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out67471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71906.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 65379_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65379_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:41:36.32 +05:28:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 0.713 3851614456442712576 145.40148019507 +05.47075544911 14.6824 14.1327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65383_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65383_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:29:01.60 +04:10:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65387_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65387_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:19:44.94 +02:36:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65390_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65390_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:25:55.73 +01:45:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65391_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65391_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:21:28.31 +09:14:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65393_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65393_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:30:46.77 +02:48:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.666 3844662862895560960 142.69533412506 +02.81235488164 14.2820 13.4958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65395_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65395_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:29:26.53 +05:40:26.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)
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Considering the candidate 65397_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65397_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:31:40.14 +02:55:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65401_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65401_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:18:43.38 +06:27:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65402_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65402_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:36:24.82 +02:47:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65403_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65403_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:34:05.50 +02:30:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65404_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 65404_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:42:41.77 +08:07:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67402_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 67402_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:10:45.07 +06:21:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67471_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
Preparing report for the candidate 67471_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
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Considering the candidate 68532_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 68532_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:14:28.57 +07:47:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68535_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 68535_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:37:17.52 +06:48:25.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 68827_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 68827_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:15:51.53 +09:00:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69586_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 69586_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:14:29.19 +02:20:22.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 70065_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 70065_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:14:25.02 +07:54:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70241_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 70241_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:22:25.95 +06:08:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70398_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 70398_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:14:28.08 +08:28:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70531_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
Preparing report for the candidate 70531_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
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Considering the candidate 70641_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 70641_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:15:11.41 +05:32:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70693_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 70693_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:15:54.05 +08:13:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70721_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 70721_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:11:55.97 +09:43:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70843_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 70843_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:23:35.72 +06:23:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70903_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 70903_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:19:43.39 +10:03:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71103_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 71103_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:21:19.66 +05:31:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71389_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 71389_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:30:01.03 +02:06:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71906_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
Preparing report for the candidate 71906_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
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Considering the candidate 72103_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 72103_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:19:53.79 +06:46:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72106_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 72106_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:27:33.97 +06:20:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72195_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 72195_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:15:21.51 +07:39:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 0.848 587093308917541504 138.83986232002 +07.65745845000 14.9036 14.4569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72355_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 72355_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:23:45.50 +10:01:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72369_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 72369_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:19:17.33 +09:58:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.187 590805706849566848 139.82240461192 +09.98020504507 14.9224 14.4311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72502_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 72502_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:11:08.83 +10:06:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 1.608 591694627640735488 137.78698916668 +10.10926446529 14.7653 14.1301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72543_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 72543_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:11:54.79 +07:55:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 2.684 590033059412994816 137.97879037137 +07.91799718650 15.7379 15.3644 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 72544_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 72544_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks
**** FOUND 09:07:52.58 +08:42:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72654_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367
The candidate 72654_fd_Hya-02-Q2b1x1_2026-04-12_23-59-46_20.00sec_-4.90C_LIGHT_0367 did not pass the final checks